1) The document reports the discovery of the first known Trojan asteroid of Earth, 2010 TK7.
2) 2010 TK7 was discovered in infrared data from the WISE spacecraft. Follow-up optical observations confirmed it is trapped in a stable orbit around the L4 Lagrangian point ahead of Earth.
3) The asteroid's orbit is stable over at least 10,000 years, though its position becomes chaotic beyond 250 years in the past or future due to gravitational interactions.
This document summarizes the discovery of two Earth-sized planets orbiting the star Kepler-20. Precise photometric data from the Kepler spacecraft revealed periodic transit signals indicating planets with sizes of 1.03 times (Kepler-20 e) and 0.87 times (Kepler-20 f) Earth's radius orbiting the star. Statistical analysis shows the planetary interpretation of the transit signals is over three orders of magnitude more likely than alternative hypotheses. The planets are likely rocky in composition.
- The International Astronomical Union reclassified Pluto from a planet to a dwarf planet due to its small size and eccentric orbit.
- Students are tasked with analyzing data about objects in the solar system to determine what characteristics qualify a body as a planet.
- The IAU decided that to be a planet, a body must orbit the sun, have a nearly circular orbit, and not cross the orbits of other planets. Students are asked if they agree with reclassifying Pluto as a dwarf planet.
IB Astrophysics - stellar distances - Flippingphysics by nothingnerdyNothingnerdy
This document discusses several methods for measuring stellar distances, including parallax, spectroscopic parallax, and Cepheid variables. Stellar parallax measures distance by observing the apparent shift in a star's position over the Earth's orbit. Spectroscopic parallax uses a star's spectrum to determine its temperature and luminosity class, allowing its distance to be estimated from models of the Hertzsprung-Russell diagram. Cepheid variables are unstable stars whose pulsation period correlates with luminosity, so observing a Cepheid's period enables its distance to be calculated. The document also defines astronomical units, light years, parsecs and absolute magnitude, which provide standardized measures of distance and brightness used in astronomy.
This chapter discusses small solar system bodies like dwarf planets, asteroids, meteoroids, comets, and Kuiper Belt objects. It describes their properties and classifications. Key points include that dwarf planets like Pluto and Eris have been discovered in the outer solar system, along with their moons. Asteroids exist in the main belt between Mars and Jupiter and some have orbits that cross Earth's. Comets contain ice and debris and have tails when close to the Sun. Impacts from these small bodies have caused mass extinctions on Earth in the past.
ILOA Galaxy Forum Europe 2013 - solar system exploration - hajime yanoILOAHawaii
The document summarizes two Japanese space missions: Hayabusa and IKAROS. Hayabusa was the first mission to return asteroid samples to Earth, rendezvousing with the asteroid Itokawa in 2005 and returning samples in 2010. It established key technologies for deep space exploration. Analysis of the Itokawa samples provided insights into asteroid composition and evolution. The IKAROS mission in 2010 demonstrated solar sail technology, the first time a solar sail propelled a spacecraft. It helped pave the way for future outer planet exploration using solar sails.
We describe the discovery of a satellite in orbit about the dwarf planet (136472) Makemake. This
satellite, provisionally designated S/2015 (136472) 1, was detected in imaging data collected with the
Hubble Space Telescope’s Wide Field Camera 3 on UTC April 27, 2015 at 7.80±0.04 magnitudes
fainter than Makemake. It likely evaded detection in previous satellite searches due to a nearly edgeon
orbital configuration, placing it deep within the glare of Makemake during a substantial fraction
of its orbital period. This configuration would place Makemake and its satellite near a mutual event
season. Insufficient orbital motion was detected to make a detailed characterization of its orbital
properties, prohibiting a measurement of the system mass with the discovery data alone. Preliminary
analysis indicates that if the orbit is circular, its orbital period must be longer than 12.4 days, and
must have a semi-major axis &21,000 km. We find that the properties of Makemake’s moon suggest
that the majority of the dark material detected in the system by thermal observations may not reside
on the surface of Makemake, but may instead be attributable to S/2015 (136472) 1 having a uniform
dark surface. This “dark moon hypothesis” can be directly tested with future JWST observations.
We discuss the implications of this discovery for the spin state, figure, and thermal properties of
Makemake and the apparent ubiquity of trans-Neptunian dwarf planet satellites.
The document presents a study using simulated type Ia supernova data to investigate how peculiar velocities affect constraints on cosmological parameters from supernova observations. The study generates a simulated supernova dataset that includes peculiar velocity information. It then constructs Hubble diagrams using true and observed redshifts from the simulations. The resulting parameter estimates are compared, finding the peculiar velocities can induce shifts in the estimated values of Ωm and H0 of approximately 1 sigma.
1. The document discusses different units used to measure astronomical distances, including the astronomical unit (AU), light year, and parsec.
2. It explains how parallax can be used to measure distances to stars by observing the apparent shift in position of a star relative to background objects as the Earth orbits the Sun.
3. Spectroscopic parallax and studying Cepheid variable stars can also be used to determine distances. Analyzing a star's spectrum provides information to estimate its luminosity and place it on the Hertzsprung-Russell diagram to find distance.
This document summarizes the discovery of two Earth-sized planets orbiting the star Kepler-20. Precise photometric data from the Kepler spacecraft revealed periodic transit signals indicating planets with sizes of 1.03 times (Kepler-20 e) and 0.87 times (Kepler-20 f) Earth's radius orbiting the star. Statistical analysis shows the planetary interpretation of the transit signals is over three orders of magnitude more likely than alternative hypotheses. The planets are likely rocky in composition.
- The International Astronomical Union reclassified Pluto from a planet to a dwarf planet due to its small size and eccentric orbit.
- Students are tasked with analyzing data about objects in the solar system to determine what characteristics qualify a body as a planet.
- The IAU decided that to be a planet, a body must orbit the sun, have a nearly circular orbit, and not cross the orbits of other planets. Students are asked if they agree with reclassifying Pluto as a dwarf planet.
IB Astrophysics - stellar distances - Flippingphysics by nothingnerdyNothingnerdy
This document discusses several methods for measuring stellar distances, including parallax, spectroscopic parallax, and Cepheid variables. Stellar parallax measures distance by observing the apparent shift in a star's position over the Earth's orbit. Spectroscopic parallax uses a star's spectrum to determine its temperature and luminosity class, allowing its distance to be estimated from models of the Hertzsprung-Russell diagram. Cepheid variables are unstable stars whose pulsation period correlates with luminosity, so observing a Cepheid's period enables its distance to be calculated. The document also defines astronomical units, light years, parsecs and absolute magnitude, which provide standardized measures of distance and brightness used in astronomy.
This chapter discusses small solar system bodies like dwarf planets, asteroids, meteoroids, comets, and Kuiper Belt objects. It describes their properties and classifications. Key points include that dwarf planets like Pluto and Eris have been discovered in the outer solar system, along with their moons. Asteroids exist in the main belt between Mars and Jupiter and some have orbits that cross Earth's. Comets contain ice and debris and have tails when close to the Sun. Impacts from these small bodies have caused mass extinctions on Earth in the past.
ILOA Galaxy Forum Europe 2013 - solar system exploration - hajime yanoILOAHawaii
The document summarizes two Japanese space missions: Hayabusa and IKAROS. Hayabusa was the first mission to return asteroid samples to Earth, rendezvousing with the asteroid Itokawa in 2005 and returning samples in 2010. It established key technologies for deep space exploration. Analysis of the Itokawa samples provided insights into asteroid composition and evolution. The IKAROS mission in 2010 demonstrated solar sail technology, the first time a solar sail propelled a spacecraft. It helped pave the way for future outer planet exploration using solar sails.
We describe the discovery of a satellite in orbit about the dwarf planet (136472) Makemake. This
satellite, provisionally designated S/2015 (136472) 1, was detected in imaging data collected with the
Hubble Space Telescope’s Wide Field Camera 3 on UTC April 27, 2015 at 7.80±0.04 magnitudes
fainter than Makemake. It likely evaded detection in previous satellite searches due to a nearly edgeon
orbital configuration, placing it deep within the glare of Makemake during a substantial fraction
of its orbital period. This configuration would place Makemake and its satellite near a mutual event
season. Insufficient orbital motion was detected to make a detailed characterization of its orbital
properties, prohibiting a measurement of the system mass with the discovery data alone. Preliminary
analysis indicates that if the orbit is circular, its orbital period must be longer than 12.4 days, and
must have a semi-major axis &21,000 km. We find that the properties of Makemake’s moon suggest
that the majority of the dark material detected in the system by thermal observations may not reside
on the surface of Makemake, but may instead be attributable to S/2015 (136472) 1 having a uniform
dark surface. This “dark moon hypothesis” can be directly tested with future JWST observations.
We discuss the implications of this discovery for the spin state, figure, and thermal properties of
Makemake and the apparent ubiquity of trans-Neptunian dwarf planet satellites.
The document presents a study using simulated type Ia supernova data to investigate how peculiar velocities affect constraints on cosmological parameters from supernova observations. The study generates a simulated supernova dataset that includes peculiar velocity information. It then constructs Hubble diagrams using true and observed redshifts from the simulations. The resulting parameter estimates are compared, finding the peculiar velocities can induce shifts in the estimated values of Ωm and H0 of approximately 1 sigma.
1. The document discusses different units used to measure astronomical distances, including the astronomical unit (AU), light year, and parsec.
2. It explains how parallax can be used to measure distances to stars by observing the apparent shift in position of a star relative to background objects as the Earth orbits the Sun.
3. Spectroscopic parallax and studying Cepheid variable stars can also be used to determine distances. Analyzing a star's spectrum provides information to estimate its luminosity and place it on the Hertzsprung-Russell diagram to find distance.
Photometry of Giant Propellers in Saturn's RingsJakaylaRobinson
1) The document discusses analyzing images of "giant propellers" in Saturn's rings taken by Cassini during its Ring Grazing Orbit and Grand Finale.
2) The authors use images of the propeller "Santos-Dumont" taken on the lit and unlit sides to investigate how the propeller's brightness relates to its optical depth, by comparing predicted and observed brightness values.
3) They find the brightness ratio between prediction and observation is consistent in translucent parts of the propeller and ring, but varies more in opaque parts, helping evaluate differences between empty and opaque regions.
This paper considers the plausibility of time dilation effects shown in the film Interstellar. It calculates that for an hour to pass on a planet orbiting a 100 million solar mass black hole while 7 years pass on Earth, the planet would need to orbit at 2.95 astronomical units from the black hole. However, this distance is inside the minimum stable orbit, so the planet would not be able to maintain that orbit around a non-rotating black hole. A rotating black hole could allow for a stable orbit at that distance. The paper also finds that travel times depicted in the film between the planet and a safe orbit are implausibly short.
This document summarizes star forming regions in the constellation of Cepheus. It describes several giant molecular cloud complexes located at various distances from the Sun, ranging from clouds within 500 pc to regions associated with the Perseus spiral arm at 2-3 kpc. Key regions discussed include the Cepheus Flare clouds below 500 pc, three OB associations (Cep OB2, Cep OB3, Cep OB4) located 600-900 pc away, and the well-known high mass star forming region S 140 located at 900 pc. Tables list molecular clouds and young stars identified in the Cepheus region. Maps show the distribution of clouds, extinction, and pre-main sequence stars across Cepheus.
This document summarizes a study examining the center of the supernova remnant SNR 0509-67.5 in the Large Magellanic Cloud to search for an ex-companion star that could distinguish between single-degenerate and double-degenerate progenitor models of Type Ia supernovae. High-resolution Hubble Space Telescope images show no point sources within the conservative 3-sigma error ellipse of the remnant's center down to a magnitude limit of V=26.9, corresponding to an absolute magnitude 4.2 magnitudes fainter than possible for any published single-degenerate model. This rules out all single-degenerate progenitor scenarios and supports a double-degenerate origin for this particular Type Ia supern
The Solar System consists of the Sun and objects bound to it by gravity, including 8 planets. The 4 inner terrestrial planets - Mercury, Venus, Earth, and Mars - are primarily rocky. The 4 outer gas giants - Jupiter, Saturn, Uranus, and Neptune - are massive and gaseous. Between Mars and Jupiter is the asteroid belt. Comets originate from the Kuiper belt beyond Neptune and have highly elliptical orbits. Each planet has unique characteristics such as atmospheric composition, rotation period, and presence of moons and rings.
UK Space Conference: James Webb Space Telescope (Gillian Wright)A. Rocketeer
The document discusses the James Webb Space Telescope, which will be the successor to the Hubble Space Telescope. It will have a 6.5 meter primary mirror, be optimized for infrared observations, and passively cooled to around 40K. The telescope will launch in June 2013 and be placed in an L2 orbit, with an expected mission lifetime of 5-10 years. It is a joint project between NASA, ESA, and the Canadian Space Agency.
The document analyzes data from the open star cluster M11 to determine its fundamental properties. Photometry of stars in M11 was performed using images taken through two filters with a telescope. A color-magnitude diagram was created and fit with theoretical models, revealing M11 to be around 250 million years old, located 5930 light years away, and having a similar iron-to-hydrogen ratio as the sun. Analysis of independent star clusters provides insights into patterns of galaxy formation and evolution.
Kepler and Newton vs. Geocentrism, Flat Earth, and the "Vortex"James Smith
This presentation compares predictions of Kepler's 3rd Law to data from almost all of the orbital systems in the Solar System (including orbits of Pluto's moons), then predicts the height of a geostationary orbit.
A rocky planet_transiting_a_nearby_low_mass_starSérgio Sacani
Um exoplaneta rochoso do tamanho da Terra, orbita uma estrela pequena e próxima, poderia ser o mundo mais importante já encontrado além do Sistema Solar, disseram os astrônomos.
O planeta localiza-se na constelação de Vela, no hemisfério sul do céu e é próximo o suficiente para que os telescópios possam observar qualquer atmosfera que ele possua, um procedimento que poderia ajudar a registrar algum tipo de vida, se ela existisse em outros planetas, no futuro.
Denominado de GJ 1132b, o exoplaneta é cerca de 16% maior que a Terra, e está localizado a cerca de 39 anos-luz de distância, o que faz com que ele seja três vezes mais próximo da Terra do que qualquer outro exoplaneta rochoso já descoberto. Nessa distância, espera-se que os telescópios sejam capazes de fazer uma análise química de sua atmosfera, a velocidade dos seus ventos e as cores do pôr-do-Sol, que acontecem no exoplaneta.
Os astrônomos registraram o planeta à medida que ele passava na frente da sua estrela, uma estrela do tipo anã vermelha, com somente um quinto do tamanho do Sol. Apesar de muito mais fria e muito mais apagada que o Sol, o GJ 1132b, tem uma órbita tão próxima da estrela que as suas temperaturas superficiais atingem cerca de 260 graus Celsius.
Essa temperatura, obviamente, é muito alta para reter a água em estado líquido na superfície do exoplaneta, fazendo com que ele seja inóspito para a vida, mas não tão quente para queimar toda uma atmosfera que pode ter se formado no planeta.
Direct imaging of exoplanets is challenging due to the small angular separation and brightness difference between planets and their host stars. The document discusses the history and recent progress of direct exoplanet imaging, including the discovery of multiple planets orbiting the star HR 8799 using adaptive optics on large telescopes. Upcoming instruments like GPI and TMT aim to directly image Earth-like exoplanets.
Galaxy Forum New York 2013 - Scarsdale - Denton EbelILOAHawaii
This document discusses asteroids, including their composition, origins, and importance for science and resources. It notes that asteroids are remnants from the early solar system and contain valuable clues about its formation. Their metals also represent important potential resources. The document outlines various asteroid missions that have enhanced scientific understanding and notes the importance of detecting potentially hazardous asteroids to prevent future impacts.
1) The document hypothesizes that dark matter images were accidentally recorded by cameras on the TSS-1R satellite during a 1996 NASA mission mishap. Disk-like images seen moving beyond the receding satellite are proposed to be evidence of dark matter.
2) It further conjectures that these disk images each represent two single-notch 2D disks "stuck together" from a lower plane of existence, representing doubled magnetic monopoles on that plane.
3) A mathematical formula is proposed to describe the number of fundamental particles ("koilon quanta") that make up electrons and other fundamental particles on different planes of existence.
Beyond the Kuiper Belt Edge: New High Perihelion Trans-Neptunian Objects With...Sérgio Sacani
We are conducting a survey for distant solar system objects beyond the Kuiper
Belt edge ( 50 AU) with new wide-field cameras on the Subaru and CTIO tele-
scopes. We are interested in the orbits of objects that are decoupled from the
giant planet region in order to understand the structure of the outer solar sys-
tem, including whether a massive planet exists beyond a few hundred AU as first
reported in Trujillo and Sheppard (2014). In addition to discovering extreme
trans-Neptunian objects detailed elsewhere, we have found several objects with
high perihelia (q > 40 AU) that differ from the extreme and inner Oort cloud
objects due to their moderate semi-major axes (50 < a < 100 AU) and eccen-
tricities (e . 0.3). Newly discovered objects 2014 FZ71 and 2015 FJ345 have
the third and fourth highest perihelia known after Sedna and 2012 VP113, yet
their orbits are not nearly as eccentric or distant. We found several of these high
perihelion but moderate orbit objects and observe that they are mostly near Nep-
tune mean motion resonances and have significant inclinations (i > 20 degrees).
These moderate objects likely obtained their unusual orbits through combined
interactions with Neptune’s mean motion resonances and the Kozai resonance,
similar to the origin scenarios for 2004 XR190. We also find the distant 2008
ST291 has likely been modified by the MMR+KR mechanism through the 6:1
Neptune resonance. We discuss these moderately eccentric, distant objects along
with some other interesting low inclination outer classical belt objects like 2012
FH84 discovered in our ongoing survey.
Visible spectra of (474640) 2004 VN112–2013 RF98 with OSIRIS at the 10.4 m GT...Sérgio Sacani
The existence of significant anisotropies in the distributions of the directions of perihelia and
orbital poles of the known extreme trans-Neptunian objects (ETNOs) has been used to claim
that trans-Plutonian planets may exist. Among the known ETNOs, the pair (474640) 2004
VN112–2013 RF98 stands out. Their orbital poles and the directions of their perihelia and their
velocities at perihelion/aphelion are separated by a few degrees, but orbital similarity does
not necessarily imply common physical origin. In an attempt to unravel their physical nature,
visible spectroscopy of both targets was obtained using the OSIRIS camera-spectrograph at the
10.4 m Gran Telescopio Canarias (GTC). From the spectral analysis, we find that 474640–2013
RF98 have similar spectral slopes (12 versus 15 per cent/0.1 µm), very different from Sedna’s
but compatible with those of (148209) 2000 CR105 and 2012 VP113. These five ETNOs belong
to the group of seven linked to the Planet Nine hypothesis. A dynamical pathway consistent
with these findings is dissociation of a binary asteroid during a close encounter with a planet
and we confirm its plausibility using N-body simulations. We thus conclude that both the
dynamical and spectroscopic properties of 474640–2013 RF98 favour a genetic link and their
current orbits suggest that the pair was kicked by a perturber near aphelion
This document analyzes over 1,000 spectra of the Beta Pictoris system obtained between 2003-2011, identifying around 6,000 variable absorption features caused by transiting exocomets. Statistical analysis reveals two distinct populations of exocomets: Population S, which produces shallow absorption lines and consists of old exhausted comets trapped in resonance with a planet; and Population D, which produces deep lines and likely results from recent fragmentation of parent bodies. Physical properties like radial velocity, line width, and orbital parameters differ between the two populations, indicating two separate families of exocomets in the Beta Pictoris system.
1. The document describes the masses, diameters, and gravitational forces of the planets in our solar system, listing them from Jupiter down to Pluto.
2. It then provides a diagram showing the relationship between the sun and the planets, with the sun's gravitational force equal to the sum of the gravitational forces of the planets.
3. The diagram also depicts the planets as waveforms in a "wave train" representing the planetary system, with the sun at one end and Pluto at the other.
Habiatal Zone (outside our solar system)Bob Smullen
The document discusses the habitability of planets outside our solar system. It covers topics like the habitable zones around different types of stars where liquid water could exist, methods used to detect exoplanets, and factors that influence a planet's potential habitability such as size, atmosphere, and distance from the host star. It also examines probabilities for life elsewhere in the galaxy based on the Drake Equation and considers challenges around detecting and communicating with intelligent civilizations.
This summarizes a scientific study on long-distance quantum teleportation between two laboratories separated by 55 meters but connected by 2 kilometers of fiber optic cable. The key points are:
1) Researchers teleported quantum states (qubits) carried by photons at 1.3 micrometer wavelengths onto photons at 1.55 micrometer wavelengths between the two laboratories.
2) The qubits were encoded in time-bin superpositions and entanglement rather than polarization to make them more robust against decoherence in optical fibers.
3) A partial Bell state measurement was performed using linear optics at the receiving end to probabilistically teleport the quantum states over the long distance.
This document provides an overview and context for a study of the symbiotic star SS Leporis using interferometric imaging with the PIONIER instrument on the VLTI. Key points:
- SS Leporis is a long-period interacting binary system composed of an A star accreting material from an evolved M giant companion, presenting an "Algol paradox" where the more evolved star is less massive.
- Previous studies have not fully constrained the system morphology and characteristics. New interferometric observations with PIONIER were obtained to directly probe the inner parts of the system.
- The observations were used to perform aperture synthesis imaging and model the system as a binary surrounded by a circumbinary disc. This provides the
Stellar Life Cycle
1. Stars are born from dense clouds of gas and dust called nebulae.
2. Most stars, including our Sun, spend the majority of their lifespan fusing hydrogen into helium as main sequence stars.
3. Towards the end of their life, stars expand into red giants or supergiants and begin fusing heavier elements, before shrinking into white dwarfs, neutron stars, or black holes.
The document discusses Sun SPOT (Small Programmable Object Technology), a small wireless sensor device developed by Sun Microsystems that runs on a Java virtual machine called Squawk. It has various sensors and I/O capabilities. The document provides details on the hardware components of Sun SPOT including its processor, radio, battery life, and sensor boards. It also describes the Squawk virtual machine and SPOT software development kit (SDK) libraries. Examples are given of interfacing SPOT with sensors, switches, LEDs, and other devices. Potential applications of Sun SPOT for wireless sensor networks are mentioned.
Photometry of Giant Propellers in Saturn's RingsJakaylaRobinson
1) The document discusses analyzing images of "giant propellers" in Saturn's rings taken by Cassini during its Ring Grazing Orbit and Grand Finale.
2) The authors use images of the propeller "Santos-Dumont" taken on the lit and unlit sides to investigate how the propeller's brightness relates to its optical depth, by comparing predicted and observed brightness values.
3) They find the brightness ratio between prediction and observation is consistent in translucent parts of the propeller and ring, but varies more in opaque parts, helping evaluate differences between empty and opaque regions.
This paper considers the plausibility of time dilation effects shown in the film Interstellar. It calculates that for an hour to pass on a planet orbiting a 100 million solar mass black hole while 7 years pass on Earth, the planet would need to orbit at 2.95 astronomical units from the black hole. However, this distance is inside the minimum stable orbit, so the planet would not be able to maintain that orbit around a non-rotating black hole. A rotating black hole could allow for a stable orbit at that distance. The paper also finds that travel times depicted in the film between the planet and a safe orbit are implausibly short.
This document summarizes star forming regions in the constellation of Cepheus. It describes several giant molecular cloud complexes located at various distances from the Sun, ranging from clouds within 500 pc to regions associated with the Perseus spiral arm at 2-3 kpc. Key regions discussed include the Cepheus Flare clouds below 500 pc, three OB associations (Cep OB2, Cep OB3, Cep OB4) located 600-900 pc away, and the well-known high mass star forming region S 140 located at 900 pc. Tables list molecular clouds and young stars identified in the Cepheus region. Maps show the distribution of clouds, extinction, and pre-main sequence stars across Cepheus.
This document summarizes a study examining the center of the supernova remnant SNR 0509-67.5 in the Large Magellanic Cloud to search for an ex-companion star that could distinguish between single-degenerate and double-degenerate progenitor models of Type Ia supernovae. High-resolution Hubble Space Telescope images show no point sources within the conservative 3-sigma error ellipse of the remnant's center down to a magnitude limit of V=26.9, corresponding to an absolute magnitude 4.2 magnitudes fainter than possible for any published single-degenerate model. This rules out all single-degenerate progenitor scenarios and supports a double-degenerate origin for this particular Type Ia supern
The Solar System consists of the Sun and objects bound to it by gravity, including 8 planets. The 4 inner terrestrial planets - Mercury, Venus, Earth, and Mars - are primarily rocky. The 4 outer gas giants - Jupiter, Saturn, Uranus, and Neptune - are massive and gaseous. Between Mars and Jupiter is the asteroid belt. Comets originate from the Kuiper belt beyond Neptune and have highly elliptical orbits. Each planet has unique characteristics such as atmospheric composition, rotation period, and presence of moons and rings.
UK Space Conference: James Webb Space Telescope (Gillian Wright)A. Rocketeer
The document discusses the James Webb Space Telescope, which will be the successor to the Hubble Space Telescope. It will have a 6.5 meter primary mirror, be optimized for infrared observations, and passively cooled to around 40K. The telescope will launch in June 2013 and be placed in an L2 orbit, with an expected mission lifetime of 5-10 years. It is a joint project between NASA, ESA, and the Canadian Space Agency.
The document analyzes data from the open star cluster M11 to determine its fundamental properties. Photometry of stars in M11 was performed using images taken through two filters with a telescope. A color-magnitude diagram was created and fit with theoretical models, revealing M11 to be around 250 million years old, located 5930 light years away, and having a similar iron-to-hydrogen ratio as the sun. Analysis of independent star clusters provides insights into patterns of galaxy formation and evolution.
Kepler and Newton vs. Geocentrism, Flat Earth, and the "Vortex"James Smith
This presentation compares predictions of Kepler's 3rd Law to data from almost all of the orbital systems in the Solar System (including orbits of Pluto's moons), then predicts the height of a geostationary orbit.
A rocky planet_transiting_a_nearby_low_mass_starSérgio Sacani
Um exoplaneta rochoso do tamanho da Terra, orbita uma estrela pequena e próxima, poderia ser o mundo mais importante já encontrado além do Sistema Solar, disseram os astrônomos.
O planeta localiza-se na constelação de Vela, no hemisfério sul do céu e é próximo o suficiente para que os telescópios possam observar qualquer atmosfera que ele possua, um procedimento que poderia ajudar a registrar algum tipo de vida, se ela existisse em outros planetas, no futuro.
Denominado de GJ 1132b, o exoplaneta é cerca de 16% maior que a Terra, e está localizado a cerca de 39 anos-luz de distância, o que faz com que ele seja três vezes mais próximo da Terra do que qualquer outro exoplaneta rochoso já descoberto. Nessa distância, espera-se que os telescópios sejam capazes de fazer uma análise química de sua atmosfera, a velocidade dos seus ventos e as cores do pôr-do-Sol, que acontecem no exoplaneta.
Os astrônomos registraram o planeta à medida que ele passava na frente da sua estrela, uma estrela do tipo anã vermelha, com somente um quinto do tamanho do Sol. Apesar de muito mais fria e muito mais apagada que o Sol, o GJ 1132b, tem uma órbita tão próxima da estrela que as suas temperaturas superficiais atingem cerca de 260 graus Celsius.
Essa temperatura, obviamente, é muito alta para reter a água em estado líquido na superfície do exoplaneta, fazendo com que ele seja inóspito para a vida, mas não tão quente para queimar toda uma atmosfera que pode ter se formado no planeta.
Direct imaging of exoplanets is challenging due to the small angular separation and brightness difference between planets and their host stars. The document discusses the history and recent progress of direct exoplanet imaging, including the discovery of multiple planets orbiting the star HR 8799 using adaptive optics on large telescopes. Upcoming instruments like GPI and TMT aim to directly image Earth-like exoplanets.
Galaxy Forum New York 2013 - Scarsdale - Denton EbelILOAHawaii
This document discusses asteroids, including their composition, origins, and importance for science and resources. It notes that asteroids are remnants from the early solar system and contain valuable clues about its formation. Their metals also represent important potential resources. The document outlines various asteroid missions that have enhanced scientific understanding and notes the importance of detecting potentially hazardous asteroids to prevent future impacts.
1) The document hypothesizes that dark matter images were accidentally recorded by cameras on the TSS-1R satellite during a 1996 NASA mission mishap. Disk-like images seen moving beyond the receding satellite are proposed to be evidence of dark matter.
2) It further conjectures that these disk images each represent two single-notch 2D disks "stuck together" from a lower plane of existence, representing doubled magnetic monopoles on that plane.
3) A mathematical formula is proposed to describe the number of fundamental particles ("koilon quanta") that make up electrons and other fundamental particles on different planes of existence.
Beyond the Kuiper Belt Edge: New High Perihelion Trans-Neptunian Objects With...Sérgio Sacani
We are conducting a survey for distant solar system objects beyond the Kuiper
Belt edge ( 50 AU) with new wide-field cameras on the Subaru and CTIO tele-
scopes. We are interested in the orbits of objects that are decoupled from the
giant planet region in order to understand the structure of the outer solar sys-
tem, including whether a massive planet exists beyond a few hundred AU as first
reported in Trujillo and Sheppard (2014). In addition to discovering extreme
trans-Neptunian objects detailed elsewhere, we have found several objects with
high perihelia (q > 40 AU) that differ from the extreme and inner Oort cloud
objects due to their moderate semi-major axes (50 < a < 100 AU) and eccen-
tricities (e . 0.3). Newly discovered objects 2014 FZ71 and 2015 FJ345 have
the third and fourth highest perihelia known after Sedna and 2012 VP113, yet
their orbits are not nearly as eccentric or distant. We found several of these high
perihelion but moderate orbit objects and observe that they are mostly near Nep-
tune mean motion resonances and have significant inclinations (i > 20 degrees).
These moderate objects likely obtained their unusual orbits through combined
interactions with Neptune’s mean motion resonances and the Kozai resonance,
similar to the origin scenarios for 2004 XR190. We also find the distant 2008
ST291 has likely been modified by the MMR+KR mechanism through the 6:1
Neptune resonance. We discuss these moderately eccentric, distant objects along
with some other interesting low inclination outer classical belt objects like 2012
FH84 discovered in our ongoing survey.
Visible spectra of (474640) 2004 VN112–2013 RF98 with OSIRIS at the 10.4 m GT...Sérgio Sacani
The existence of significant anisotropies in the distributions of the directions of perihelia and
orbital poles of the known extreme trans-Neptunian objects (ETNOs) has been used to claim
that trans-Plutonian planets may exist. Among the known ETNOs, the pair (474640) 2004
VN112–2013 RF98 stands out. Their orbital poles and the directions of their perihelia and their
velocities at perihelion/aphelion are separated by a few degrees, but orbital similarity does
not necessarily imply common physical origin. In an attempt to unravel their physical nature,
visible spectroscopy of both targets was obtained using the OSIRIS camera-spectrograph at the
10.4 m Gran Telescopio Canarias (GTC). From the spectral analysis, we find that 474640–2013
RF98 have similar spectral slopes (12 versus 15 per cent/0.1 µm), very different from Sedna’s
but compatible with those of (148209) 2000 CR105 and 2012 VP113. These five ETNOs belong
to the group of seven linked to the Planet Nine hypothesis. A dynamical pathway consistent
with these findings is dissociation of a binary asteroid during a close encounter with a planet
and we confirm its plausibility using N-body simulations. We thus conclude that both the
dynamical and spectroscopic properties of 474640–2013 RF98 favour a genetic link and their
current orbits suggest that the pair was kicked by a perturber near aphelion
This document analyzes over 1,000 spectra of the Beta Pictoris system obtained between 2003-2011, identifying around 6,000 variable absorption features caused by transiting exocomets. Statistical analysis reveals two distinct populations of exocomets: Population S, which produces shallow absorption lines and consists of old exhausted comets trapped in resonance with a planet; and Population D, which produces deep lines and likely results from recent fragmentation of parent bodies. Physical properties like radial velocity, line width, and orbital parameters differ between the two populations, indicating two separate families of exocomets in the Beta Pictoris system.
1. The document describes the masses, diameters, and gravitational forces of the planets in our solar system, listing them from Jupiter down to Pluto.
2. It then provides a diagram showing the relationship between the sun and the planets, with the sun's gravitational force equal to the sum of the gravitational forces of the planets.
3. The diagram also depicts the planets as waveforms in a "wave train" representing the planetary system, with the sun at one end and Pluto at the other.
Habiatal Zone (outside our solar system)Bob Smullen
The document discusses the habitability of planets outside our solar system. It covers topics like the habitable zones around different types of stars where liquid water could exist, methods used to detect exoplanets, and factors that influence a planet's potential habitability such as size, atmosphere, and distance from the host star. It also examines probabilities for life elsewhere in the galaxy based on the Drake Equation and considers challenges around detecting and communicating with intelligent civilizations.
This summarizes a scientific study on long-distance quantum teleportation between two laboratories separated by 55 meters but connected by 2 kilometers of fiber optic cable. The key points are:
1) Researchers teleported quantum states (qubits) carried by photons at 1.3 micrometer wavelengths onto photons at 1.55 micrometer wavelengths between the two laboratories.
2) The qubits were encoded in time-bin superpositions and entanglement rather than polarization to make them more robust against decoherence in optical fibers.
3) A partial Bell state measurement was performed using linear optics at the receiving end to probabilistically teleport the quantum states over the long distance.
This document provides an overview and context for a study of the symbiotic star SS Leporis using interferometric imaging with the PIONIER instrument on the VLTI. Key points:
- SS Leporis is a long-period interacting binary system composed of an A star accreting material from an evolved M giant companion, presenting an "Algol paradox" where the more evolved star is less massive.
- Previous studies have not fully constrained the system morphology and characteristics. New interferometric observations with PIONIER were obtained to directly probe the inner parts of the system.
- The observations were used to perform aperture synthesis imaging and model the system as a binary surrounded by a circumbinary disc. This provides the
Stellar Life Cycle
1. Stars are born from dense clouds of gas and dust called nebulae.
2. Most stars, including our Sun, spend the majority of their lifespan fusing hydrogen into helium as main sequence stars.
3. Towards the end of their life, stars expand into red giants or supergiants and begin fusing heavier elements, before shrinking into white dwarfs, neutron stars, or black holes.
The document discusses Sun SPOT (Small Programmable Object Technology), a small wireless sensor device developed by Sun Microsystems that runs on a Java virtual machine called Squawk. It has various sensors and I/O capabilities. The document provides details on the hardware components of Sun SPOT including its processor, radio, battery life, and sensor boards. It also describes the Squawk virtual machine and SPOT software development kit (SDK) libraries. Examples are given of interfacing SPOT with sensors, switches, LEDs, and other devices. Potential applications of Sun SPOT for wireless sensor networks are mentioned.
The document announces a series of campus ambassador demos at the University of Melbourne on topics related to SunSPOT technology, Netbeans IDE, and Java application development. Soft drinks and pizza will be provided at the demos. Interested parties are instructed to RSVP by email. Additional details are given on SunSPOT hardware, the Squawk Java virtual machine, and developing applications for SunSPOT. Attendees can learn more about Sun certification opportunities.
This document provides an overview of Hubble Space Telescope images, organized into 25 chapters on astronomical subjects. It begins with an introduction describing Hubble's launch and key accomplishments over 25 years of operation. The chapters then each describe a notable Hubble image, including details revealed in the image and related scientific discoveries. Subjects range from planets in the solar system to distant galaxies. The document concludes by recognizing Hubble's ongoing contributions to astronomy through unprecedented views of the universe.
The Orion Nebula is an emission nebula located in the constellation Orion where stars are actively forming. It is approximately 1,500 light years from Earth. The nebula contains the Trapezium cluster, which has four massive stars at its center that help illuminate the nebula. Scientists recently discovered a potential black hole at the center of the Trapezium cluster that is about 200 times the mass of our Sun and helps explain the motion and evolution of stars in the Orion Nebula.
Rubric evaluation media instructional k7alatifgapor
This document provides a rubric for evaluating instructional materials. The rubric contains 10 rating areas: alignment with standards, accurate information, age-appropriate language, interest/engagement, technical quality, ease of use, lack of bias, user guide/directions, variety of media, and multisensory experience. Each area is rated on a scale of 1 to 3, with 3 being high quality and 1 being low quality. The rubric defines what constitutes a rating of 1, 2, or 3 for each of the 10 areas.
This document summarizes stellar evolution and the life cycles of stars. It describes how stars are born from nebulae and discusses the stages stars pass through, including their time as main sequence stars fueled by hydrogen fusion. As stars age and exhaust their hydrogen, they evolve into red giants and later planetary nebulae, leaving behind white dwarf cores. More massive stars explode as supernovae, forming neutron stars or black holes. Key concepts covered include nucleosynthesis, variable stars, and the end states of small and massive stars.
Stars form from dense regions in nebulae where dust and gases heat up and contract to form a protostar with enough mass for nuclear fusion to begin. Most stars will spend around 90% of their life as a main sequence star stably fusing hydrogen into helium. A star's mass determines its place on the main sequence, with smaller, cooler red stars living the longest. Lower mass stars eventually become white dwarfs as their cores grow without outward pressure, while higher mass stars explode as supernovae, leaving behind neutron stars or black holes if the core is massive enough for its surface gravity to trap even light.
This document contains descriptions of various astronomical objects and natural landscapes that are presented as reflections of God's creation. These include nebulae like the Great Carina Nebula, star clusters like R136, galaxies like the Andromeda Galaxy, planetary objects like Jupiter, terrestrial landscapes from Canada and more. The document expresses appreciation for God's creation and an encouragement to be good stewards of it.
Instructional materials are tools used by teachers to help students learn, including resources for active learning and assessment. There are many types of instructional materials classified as visual, audio, audiovisual, printed, software, equipment, electronic, non-projected, two-dimensional, and three-dimensional materials. Instructional materials make teaching easier by gaining student attention, highlighting key points, stimulating understanding, and providing shared learning experiences.
A nebula is an interstellar cloud of dust, gas, and plasma that is the first stage of star formation. Nebulae form from the gravitational collapse of gas clouds in space. As gas and dust clump together in nebulae, it can form stars and planetary systems. Some nebulae are formed from stellar explosions like supernovae, which throw off ionized material that glows.
Nebulae consist of gas and dust clouds where stars are born. Stars spend most of their lives on the main sequence, fusing hydrogen into helium in their cores. Eventually they run out of fuel and die, either exploding as supernovae or shedding their outer layers as planetary nebulae. What remains depends on the star's mass - it can become a neutron star, black hole, or white dwarf.
I. Interstellar Medium refers to the gas and dust between stars.
II. A nebula is a dense cloud of dust and gases that begins to contract due to gravity, increasing pressure and temperature to form a protostar.
III. When the protostar gets hot enough, fusion begins and a main sequence star is born.
Completing the learning experience: Instructional materialsDea Timbreza
An introduction to Instructional Materials. Presented at the Jose Rizal University Graduate school last trimester.
Subject: Production and Testing of Materials
This document discusses instructional materials used in education. It begins by outlining the learner objectives of being able to identify variables in selecting instructional materials, cite the components required to effectively communicate, and discuss general principles. It then defines instructional materials and their purpose in helping communicate information and improve student abilities. The three major components of instructional materials are identified as the delivery system, content, and presentation. Various types of written instructional materials like handouts, leaflets, books and pamphlets are discussed along with their advantages and disadvantages. The steps in developing learning resource materials and commercially prepared materials are also outlined.
Stars are luminous spheres of plasma held together by gravity that produce heat, light, and radiation. They are composed largely of gas and plasma and are responsible for distributing heavy elements throughout the universe. The nearest star to Earth is our Sun. Constellations are specific areas of the celestial sphere defined by groups of prominent stars that make identifiable patterns, with some famous examples being Orion and Cassiopeia.
Selection and preparation of instructional materialsMits
This document discusses the selection and preparation of instructional materials for teaching. It identifies different types of media resources that can be used, including audio visual, non-projected visual, projected visual, audio media, films and videos, and simulation and gaming. Some specific examples of materials provided are chalkboards, overhead projectors, slides, audio tapes, textbooks, and workbooks. The document outlines general principles for selecting instructional materials, such as choosing materials that are appropriate for the learning activities and styles of students.
A super earth transiting a naked-eye starSérgio Sacani
This document summarizes the detection of transits of an exoplanet orbiting the star 55 Cnc, using photometry from the MOST space telescope. The transits match the period, phase, duration, and depth predicted for the innermost planet of 55 Cnc, designated 55 Cnc e. Analysis of the transit data indicates the planet has a mass of 8.57 Earth masses, a radius of 1.63 Earth radii, and a dense composition of rock and iron. This makes 55 Cnc e similar to other dense super-Earth exoplanets in short orbits, unlike lower-density super-Earths further from their stars. The brightness of 55 Cnc will enable further study of this transiting exoplanet system.
Pluto orbits beyond the orbit of neptuneJoyce Nael
Pluto orbits beyond Neptune and is classified as a dwarf planet. It is much smaller than Earth's moon. Pluto has a diameter of 2,274 km and its orbit averages 39.5 AU from the sun. Pluto was discovered in 1930 and named after the Roman god of the underworld. It has a large moon called Charon about half its size. The discovery of additional Kuiper belt objects and debate over its classification led to Pluto being reclassified as a dwarf planet in 2006.
The document discusses the 20-year history and impact of the Hubble Space Telescope. Key points include: (1) Hubble was launched in 1990 and has been serviced multiple times to increase its lifespan, with a final servicing in 2009; (2) It has greatly improved imaging quality over its lifetime and increased our understanding of galaxies, stars and planetary formation; (3) Hubble has made groundbreaking discoveries like observing comet Shoemaker-Levy's impact on Jupiter and helped capture humanity's imagination about space.
Analysis of most_light_curves_of_five_young_stars_in_taurus_auriga_and_lupus_3...Sérgio Sacani
This document analyzes light curves from the MOST satellite of five young stars in star-forming regions. Light curves of three spotted weak-line T Tauri stars (V410 Tau, V987 Tau, and Lupus 3-14) show small values of the solar-type differential rotation parameter, indicating slightly non-rigid rotation. Light curves of another spotted weak-line T Tauri star (Lupus 3-48) are consistent with rigid rotation. Three similar flares were detected in the light curve of Lupus 3-14. The light curve of the classical T Tauri star RY Tau showed continuous decreasing brightness over three weeks of observation with variable modulation and no obvious periodic signal.
This document summarizes observations of the debris disk around the subgiant star κ CrB using Herschel and Keck. Herschel spatially resolved images of the debris disk, the first such images of a disk around a subgiant star. Keck radial velocity monitoring provided evidence for a second planetary companion around κ CrB. Keck adaptive optics imaging placed an upper limit on the mass of this companion. Modeling of the Herschel images showed the dust is broadly distributed but could not distinguish between a single wide belt or two narrow belts. The observations are consistent with dynamical depletion or collisional erosion clearing the inner regions of the disk.
The 12 biggest objects in the universe presented in a 5 inch screen, how crazy is that?. Be amazed of what the universe holds, be ready to blow your minds.
1. The document describes the motions of objects in the sky and our location in the universe, including a description of the Milky Way galaxy and our solar system.
2. Key concepts covered include the coordinate systems used to locate celestial objects, precession of the Earth, and the causes of the seasons due to the tilt of the Earth's axis.
3. Motions of objects like the sun and stars are explained, including how the sun appears to move along the ecliptic and causes the seasons as the Earth orbits around it.
Plutino an accidental_quasi-satellite_of_plutoSérgio Sacani
Plutino 15810 (1994 JR1) is currently in a 1:1 mean motion resonance with Pluto, following a quasi-satellite path where its mean longitude circulates with a superimposed libration. N-body simulations show it will remain in this quasi-satellite state, where it moves around Pluto like a retrograde satellite but with a non-closed trajectory, for nearly 350,000 years. This makes 15810 the first known minor body in a 1:1 resonance with Pluto and the first quasi-satellite discovered in the trans-Neptunian region. The quasi-satellite behavior is triggered by the object's 2:3 mean motion resonance with Neptune.
Plutino an accidental_quasi-satellite_of_plutoSérgio Sacani
1) Plutino 15810 (1994 JR1) is currently in a 1:1 mean motion resonance with Pluto, following a quasi-satellite path where its mean longitude circulates with a superimposed libration.
2) Numerical simulations show that 15810 will remain in this quasi-satellite state for nearly 350,000 years, making it the first known quasi-satellite of Pluto.
3) Pluto is the second dwarf planet after Ceres found to host a quasi-satellite. The discovery of 15810 confirms that quasi-satellite resonant states can exist for dwarf planets and asteroids.
Ingrid Stairs: PSR B1620-26 and the Methuselah Planet*JeremyHeyl
This document summarizes research on the millisecond pulsar PSR B1620-26 and its planetary system. Key points include:
- PSR B1620-26 has an inner orbit with a white dwarf companion and an outer orbit with a planetary companion in a wide, eccentric orbit.
- Timing data from 2001-2009 showed an anomaly that disrupted modeling of the dual-Keplerian orbits. Current research aims to fit a full 3-body numerical model to explain this.
- The planetary companion has a mass of about 2.5 Jupiter masses and orbits every 60-1200 years. The white dwarf companion is undermassive and young, at 480 million years old.
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Project about Pluto for Planetary Geology 2010
I updated some information and pictures on this powerpoint on 10/16/12
http://www.youtube.com/watch?v=HEheh1BH34Q
1) The Oort cloud is believed to lie at the edge of our solar system, between 5,000 and 100,000 AU from the sun, and is composed of icy objects and long-period comets.
2) Voyager 1 was the first human-made object to leave the solar system in 2012 when it crossed the heliopause and entered interstellar space.
3) Recent discoveries of objects Sedna and 2012 VP113 in the inner Oort cloud provide insights into the formation and edge of the solar system.
Dark side ofthe_universe_public_29_september_2017_nazarbayev_shrtZhaksylyk Kazykenov
1) The document discusses the history of discoveries about the universe, from ancient cosmologies to modern precision cosmology. Key developments include realizing the sun is at the center of the solar system, discovering other galaxies and the expansion of the universe, and detecting the cosmic microwave background and dark matter.
2) Current open questions about the universe include the nature of dark matter and dark energy. Observations show dark energy is accelerating the expansion of the universe, but its underlying cause remains unknown. Precise measurements aim to distinguish between models of dark energy.
3) The standard cosmological model has been very successful in explaining observations but has fine-tuning problems regarding why the present epoch is dominated by both matter and dark energy.
Planetesimal ejection describes how leftover debris from the formation of the planets was captured as moons or ended up in the asteroid belt, Kuiper belt, or Oort cloud. Asteroids and meteoroids are small rocky or metallic objects found primarily in the inner solar system, with asteroids larger than 100 meters and meteoroids smaller. They orbit near the plane of the solar system in regions like the asteroid belt. When these objects enter the Earth's atmosphere, they appear as meteors and some survive impact as meteorites. Larger impacts are rarer but can cause global effects like the extinction of dinosaurs.
Small dust particles escaping from Pluto's moons Nix and Hydra could temporarily form a ring around Pluto due to impacts, but the solar radiation pressure would remove about half of 1 micrometer particles within a year by causing collisions with Pluto and its moons. Numerical simulations found that a tenuous ring with an optical depth of 6×10^-11 could be maintained by dust released from Nix and Hydra.
A Tale of 3 Dwarf Planets: Ices and Organics on Sedna, Gonggong, and Quaoar f...Sérgio Sacani
The dwarf planets Sedna, Gonggong, and Quaoar are interesting in being somewhat smaller than
the methane-rich bodies of the Kuiper Belt (Pluto, Eris, Makemake), yet large enough to be
spherical and to have possibly undergone interior melting and differentiation. They also reside
on very different orbits, making them an ideal suite of bodies for untangling effects of size and
orbit on present day surface composition. We observed Sedna, Gonggong, and Quaoar with the
NIRSpec instrument on the James Webb Space Telescope (JWST). All three bodies were
observed in the low-resolution prism mode at wavelengths spanning 0.7 to 5.2 μm. Quaoar was
additionally observed at 10x higher spectral resolution from 0.97 to 3.16 μm using mediumresolution gratings. Sedna’s spectrum shows a large number of absorption features due to ethane
(C2H6), as well as acetylene (C2H2), ethylene (C2H4), H2O, and possibly minor CO2.
Gonggong’s spectrum also shows several, but fewer and weaker, ethane features, along with
stronger and cleaner H2O features and CO2 complexed with other molecules. Quaoar’s prism
spectrum shows even fewer and weaker ethane features, the deepest and cleanest H2O features, a
feature at 3.2 μm possibly due to HCN, and CO2 ice. The higher-resolution medium grating
spectrum of Quaoar reveals several overtone and combination bands of ethane and methane
(CH4). Spectra of all three objects show steep red spectral slopes and strong, broad absorptions
between 2.7 and 3.6 μm indicative of complex organic molecules. The suite of light
hydrocarbons and complex organic molecules are interpreted as the products of irradiation of
methane. The differences in apparent abundances of irradiation products among these three
similarly-sized bodies are likely due to their distinctive orbits, which lead to different timescales
of methane retention and to different charged particle irradiation environments. In all cases,
however, the continued presence of light hydrocarbons implies a resupply of methane to the
2
surface. We suggest that these three bodies have undergone internal melting and geochemical
evolution similar to the larger dwarf planets and distinct from all smaller KBOs. The feature
identification presented in this paper is the first step of analysis, and additional insight into the
relative abundances and mixing states of materials on these surfaces will come from future
spectral modeling of these data.
This document summarizes the detection of a super-Earth planet orbiting the star GJ 832. Radial velocity data from three telescopes revealed a planet, GJ 832c, with an orbital period of 35.68 days and a minimum mass of 5.4 Earth masses. GJ 832c has a low eccentricity orbit of 0.18 near the inner edge of the star's habitable zone. However, given its large mass, the planet likely has a massive atmosphere that could render it uninhabitable. The GJ 832 system resembles a miniature version of our solar system, with an interior potentially rocky planet and a distant gas giant.
1. VFTS 682 is a very massive star located 29 pc in projection from the young massive cluster R136 in the Tarantula Nebula of the LMC.
2. Spectral modeling finds it has an unusually high luminosity of log(L/L) = 6.5, corresponding to a present-day mass of ~150 solar masses.
3. Its isolation and mass pose the question of whether it formed in situ, which would profoundly impact theories of massive star formation, or if it was ejected from R136, making it the most massive runaway star known.
This document introduces the VLT-FLAMES Tarantula Survey, which obtained multi-epoch optical spectroscopy of over 800 massive stars in the 30 Doradus region of the Large Magellanic Cloud. The survey aims to detect massive binary systems through variations in radial velocities and to characterize the properties of O- and B-type stars, addressing questions about stellar and cluster evolution. Spectral classifications are provided for newly discovered emission-line stars, including a new Wolf-Rayet star. The survey data and reduction procedures are overviewed, and upcoming analyses of the massive star properties are announced.
The binding of cosmological structures by massless topological defectsSérgio Sacani
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field
equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational
field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin
spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling
concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect
light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is
mitigated, at least in part.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Tr...Sérgio Sacani
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the
atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets
receiving low insolation is still small, limiting our ability to understand the diversity of the atmospheric
composition and climates of temperate terrestrial planets. We report the discovery of an Earth-sized planet
transiting the nearby (12 pc) inactive M3.0 dwarf Gliese 12 (TOI-6251) with an orbital period (Porb) of 12.76 days.
The planet, Gliese 12 b, was initially identified as a candidate with an ambiguous Porb from TESS data. We
confirmed the transit signal and Porb using ground-based photometry with MuSCAT2 and MuSCAT3, and
validated the planetary nature of the signal using high-resolution images from Gemini/NIRI and Keck/NIRC2 as
well as radial velocity (RV) measurements from the InfraRed Doppler instrument on the Subaru 8.2 m telescope
and from CARMENES on the CAHA 3.5 m telescope. X-ray observations with XMM-Newton showed the host
star is inactive, with an X-ray-to-bolometric luminosity ratio of log 5.7 L L X bol » - . Joint analysis of the light
curves and RV measurements revealed that Gliese 12 b has a radius of 0.96 ± 0.05 R⊕,a3σ mass upper limit of
3.9 M⊕, and an equilibrium temperature of 315 ± 6 K assuming zero albedo. The transmission spectroscopy metric
(TSM) value of Gliese 12 b is close to the TSM values of the TRAPPIST-1 planets, adding Gliese 12 b to the small
list of potentially terrestrial, temperate planets amenable to atmospheric characterization with JWST.
Gliese 12 b, a temperate Earth-sized planet at 12 parsecs discovered with TES...Sérgio Sacani
We report on the discovery of Gliese 12 b, the nearest transiting temperate, Earth-sized planet found to date. Gliese 12 is a
bright (V = 12.6 mag, K = 7.8 mag) metal-poor M4V star only 12.162 ± 0.005 pc away from the Solar system with one of the
lowest stellar activity levels known for M-dwarfs. A planet candidate was detected by TESS based on only 3 transits in sectors
42, 43, and 57, with an ambiguity in the orbital period due to observational gaps. We performed follow-up transit observations
with CHEOPS and ground-based photometry with MINERVA-Australis, SPECULOOS, and Purple Mountain Observatory,
as well as further TESS observations in sector 70. We statistically validate Gliese 12 b as a planet with an orbital period of
12.76144 ± 0.00006 d and a radius of 1.0 ± 0.1 R⊕, resulting in an equilibrium temperature of ∼315 K. Gliese 12 b has excellent
future prospects for precise mass measurement, which may inform how planetary internal structure is affected by the stellar
compositional environment. Gliese 12 b also represents one of the best targets to study whether Earth-like planets orbiting cool
stars can retain their atmospheres, a crucial step to advance our understanding of habitability on Earth and across the galaxy.
The importance of continents, oceans and plate tectonics for the evolution of...Sérgio Sacani
Within the uncertainties of involved astronomical and biological parameters, the Drake Equation
typically predicts that there should be many exoplanets in our galaxy hosting active, communicative
civilizations (ACCs). These optimistic calculations are however not supported by evidence, which is
often referred to as the Fermi Paradox. Here, we elaborate on this long-standing enigma by showing
the importance of planetary tectonic style for biological evolution. We summarize growing evidence
that a prolonged transition from Mesoproterozoic active single lid tectonics (1.6 to 1.0 Ga) to modern
plate tectonics occurred in the Neoproterozoic Era (1.0 to 0.541 Ga), which dramatically accelerated
emergence and evolution of complex species. We further suggest that both continents and oceans
are required for ACCs because early evolution of simple life must happen in water but late evolution
of advanced life capable of creating technology must happen on land. We resolve the Fermi Paradox
(1) by adding two additional terms to the Drake Equation: foc
(the fraction of habitable exoplanets
with significant continents and oceans) and fpt
(the fraction of habitable exoplanets with significant
continents and oceans that have had plate tectonics operating for at least 0.5 Ga); and (2) by
demonstrating that the product of foc
and fpt
is very small (< 0.00003–0.002). We propose that the lack
of evidence for ACCs reflects the scarcity of long-lived plate tectonics and/or continents and oceans on
exoplanets with primitive life.
A Giant Impact Origin for the First Subduction on EarthSérgio Sacani
Hadean zircons provide a potential record of Earth's earliest subduction 4.3 billion years ago. Itremains enigmatic how subduction could be initiated so soon after the presumably Moon‐forming giant impact(MGI). Earlier studies found an increase in Earth's core‐mantle boundary (CMB) temperature due to theaccumulation of the impactor's core, and our recent work shows Earth's lower mantle remains largely solid, withsome of the impactor's mantle potentially surviving as the large low‐shear velocity provinces (LLSVPs). Here,we show that a hot post‐impact CMB drives the initiation of strong mantle plumes that can induce subductioninitiation ∼200 Myr after the MGI. 2D and 3D thermomechanical computations show that a high CMBtemperature is the primary factor triggering early subduction, with enrichment of heat‐producing elements inLLSVPs as another potential factor. The models link the earliest subduction to the MGI with implications forunderstanding the diverse tectonic regimes of rocky planets.
Climate extremes likely to drive land mammal extinction during next supercont...Sérgio Sacani
Mammals have dominated Earth for approximately 55 Myr thanks to their
adaptations and resilience to warming and cooling during the Cenozoic. All
life will eventually perish in a runaway greenhouse once absorbed solar
radiation exceeds the emission of thermal radiation in several billions of
years. However, conditions rendering the Earth naturally inhospitable to
mammals may develop sooner because of long-term processes linked to
plate tectonics (short-term perturbations are not considered here). In
~250 Myr, all continents will converge to form Earth’s next supercontinent,
Pangea Ultima. A natural consequence of the creation and decay of Pangea
Ultima will be extremes in pCO2 due to changes in volcanic rifting and
outgassing. Here we show that increased pCO2, solar energy (F⨀;
approximately +2.5% W m−2 greater than today) and continentality (larger
range in temperatures away from the ocean) lead to increasing warming
hostile to mammalian life. We assess their impact on mammalian
physiological limits (dry bulb, wet bulb and Humidex heat stress indicators)
as well as a planetary habitability index. Given mammals’ continued survival,
predicted background pCO2 levels of 410–816 ppm combined with increased
F⨀ will probably lead to a climate tipping point and their mass extinction.
The results also highlight how global landmass configuration, pCO2 and F⨀
play a critical role in planetary habitability.
Constraints on Neutrino Natal Kicks from Black-Hole Binary VFTS 243Sérgio Sacani
The recently reported observation of VFTS 243 is the first example of a massive black-hole binary
system with negligible binary interaction following black-hole formation. The black-hole mass (≈10M⊙)
and near-circular orbit (e ≈ 0.02) of VFTS 243 suggest that the progenitor star experienced complete
collapse, with energy-momentum being lost predominantly through neutrinos. VFTS 243 enables us to
constrain the natal kick and neutrino-emission asymmetry during black-hole formation. At 68% confidence
level, the natal kick velocity (mass decrement) is ≲10 km=s (≲1.0M⊙), with a full probability distribution
that peaks when ≈0.3M⊙ were ejected, presumably in neutrinos, and the black hole experienced a natal
kick of 4 km=s. The neutrino-emission asymmetry is ≲4%, with best fit values of ∼0–0.2%. Such a small
neutrino natal kick accompanying black-hole formation is in agreement with theoretical predictions.
Detectability of Solar Panels as a TechnosignatureSérgio Sacani
In this work, we assess the potential detectability of solar panels made of silicon on an Earth-like
exoplanet as a potential technosignature. Silicon-based photovoltaic cells have high reflectance in the
UV-VIS and in the near-IR, within the wavelength range of a space-based flagship mission concept
like the Habitable Worlds Observatory (HWO). Assuming that only solar energy is used to provide
the 2022 human energy needs with a land cover of ∼ 2.4%, and projecting the future energy demand
assuming various growth-rate scenarios, we assess the detectability with an 8 m HWO-like telescope.
Assuming the most favorable viewing orientation, and focusing on the strong absorption edge in the
ultraviolet-to-visible (0.34 − 0.52 µm), we find that several 100s of hours of observation time is needed
to reach a SNR of 5 for an Earth-like planet around a Sun-like star at 10pc, even with a solar panel
coverage of ∼ 23% land coverage of a future Earth. We discuss the necessity of concepts like Kardeshev
Type I/II civilizations and Dyson spheres, which would aim to harness vast amounts of energy. Even
with much larger populations than today, the total energy use of human civilization would be orders of
magnitude below the threshold for causing direct thermal heating or reaching the scale of a Kardashev
Type I civilization. Any extraterrrestrial civilization that likewise achieves sustainable population
levels may also find a limit on its need to expand, which suggests that a galaxy-spanning civilization
as imagined in the Fermi paradox may not exist.
Jet reorientation in central galaxies of clusters and groups: insights from V...Sérgio Sacani
Recent observations of galaxy clusters and groups with misalignments between their central AGN jets
and X-ray cavities, or with multiple misaligned cavities, have raised concerns about the jet – bubble
connection in cooling cores, and the processes responsible for jet realignment. To investigate the
frequency and causes of such misalignments, we construct a sample of 16 cool core galaxy clusters and
groups. Using VLBA radio data we measure the parsec-scale position angle of the jets, and compare
it with the position angle of the X-ray cavities detected in Chandra data. Using the overall sample
and selected subsets, we consistently find that there is a 30% – 38% chance to find a misalignment
larger than ∆Ψ = 45◦ when observing a cluster/group with a detected jet and at least one cavity. We
determine that projection may account for an apparently large ∆Ψ only in a fraction of objects (∼35%),
and given that gas dynamical disturbances (as sloshing) are found in both aligned and misaligned
systems, we exclude environmental perturbation as the main driver of cavity – jet misalignment.
Moreover, we find that large misalignments (up to ∼ 90◦
) are favored over smaller ones (45◦ ≤ ∆Ψ ≤
70◦
), and that the change in jet direction can occur on timescales between one and a few tens of Myr.
We conclude that misalignments are more likely related to actual reorientation of the jet axis, and we
discuss several engine-based mechanisms that may cause these dramatic changes.
The solar dynamo begins near the surfaceSérgio Sacani
The magnetic dynamo cycle of the Sun features a distinct pattern: a propagating
region of sunspot emergence appears around 30° latitude and vanishes near the
equator every 11 years (ref. 1). Moreover, longitudinal flows called torsional oscillations
closely shadow sunspot migration, undoubtedly sharing a common cause2. Contrary
to theories suggesting deep origins of these phenomena, helioseismology pinpoints
low-latitude torsional oscillations to the outer 5–10% of the Sun, the near-surface
shear layer3,4. Within this zone, inwardly increasing differential rotation coupled with
a poloidal magnetic field strongly implicates the magneto-rotational instability5,6,
prominent in accretion-disk theory and observed in laboratory experiments7.
Together, these two facts prompt the general question: whether the solar dynamo is
possibly a near-surface instability. Here we report strong affirmative evidence in stark
contrast to traditional models8 focusing on the deeper tachocline. Simple analytic
estimates show that the near-surface magneto-rotational instability better explains
the spatiotemporal scales of the torsional oscillations and inferred subsurface
magnetic field amplitudes9. State-of-the-art numerical simulations corroborate these
estimates and reproduce hemispherical magnetic current helicity laws10. The dynamo
resulting from a well-understood near-surface phenomenon improves prospects
for accurate predictions of full magnetic cycles and space weather, affecting the
electromagnetic infrastructure of Earth.
Extensive Pollution of Uranus and Neptune’s Atmospheres by Upsweep of Icy Mat...Sérgio Sacani
In the Nice model of solar system formation, Uranus and Neptune undergo an orbital upheaval,
sweeping through a planetesimal disk. The region of the disk from which material is accreted by
the ice giants during this phase of their evolution has not previously been identified. We perform
direct N-body orbital simulations of the four giant planets to determine the amount and origin of solid
accretion during this orbital upheaval. We find that the ice giants undergo an extreme bombardment
event, with collision rates as much as ∼3 per hour assuming km-sized planetesimals, increasing the
total planet mass by up to ∼0.35%. In all cases, the initially outermost ice giant experiences the
largest total enhancement. We determine that for some plausible planetesimal properties, the resulting
atmospheric enrichment could potentially produce sufficient latent heat to alter the planetary cooling
timescale according to existing models. Our findings suggest that substantial accretion during this
phase of planetary evolution may have been sufficient to impact the atmospheric composition and
thermal evolution of the ice giants, motivating future work on the fate of deposited solid material.
Exomoons & Exorings with the Habitable Worlds Observatory I: On the Detection...Sérgio Sacani
The highest priority recommendation of the Astro2020 Decadal Survey for space-based astronomy
was the construction of an observatory capable of characterizing habitable worlds. In this paper series
we explore the detectability of and interference from exomoons and exorings serendipitously observed
with the proposed Habitable Worlds Observatory (HWO) as it seeks to characterize exoplanets, starting
in this manuscript with Earth-Moon analog mutual events. Unlike transits, which only occur in systems
viewed near edge-on, shadow (i.e., solar eclipse) and lunar eclipse mutual events occur in almost every
star-planet-moon system. The cadence of these events can vary widely from ∼yearly to multiple events
per day, as was the case in our younger Earth-Moon system. Leveraging previous space-based (EPOXI)
lightcurves of a Moon transit and performance predictions from the LUVOIR-B concept, we derive
the detectability of Moon analogs with HWO. We determine that Earth-Moon analogs are detectable
with observation of ∼2-20 mutual events for systems within 10 pc, and larger moons should remain
detectable out to 20 pc. We explore the extent to which exomoon mutual events can mimic planet
features and weather. We find that HWO wavelength coverage in the near-IR, specifically in the 1.4 µm
water band where large moons can outshine their host planet, will aid in differentiating exomoon signals
from exoplanet variability. Finally, we predict that exomoons formed through collision processes akin
to our Moon are more likely to be detected in younger systems, where shorter orbital periods and
favorable geometry enhance the probability and frequency of mutual events.
Emergent ribozyme behaviors in oxychlorine brines indicate a unique niche for...Sérgio Sacani
Mars is a particularly attractive candidate among known astronomical objects
to potentially host life. Results from space exploration missions have provided
insights into Martian geochemistry that indicate oxychlorine species, particularly perchlorate, are ubiquitous features of the Martian geochemical landscape. Perchlorate presents potential obstacles for known forms of life due to
its toxicity. However, it can also provide potential benefits, such as producing
brines by deliquescence, like those thought to exist on present-day Mars. Here
we show perchlorate brines support folding and catalysis of functional RNAs,
while inactivating representative protein enzymes. Additionally, we show
perchlorate and other oxychlorine species enable ribozyme functions,
including homeostasis-like regulatory behavior and ribozyme-catalyzed
chlorination of organic molecules. We suggest nucleic acids are uniquely wellsuited to hypersaline Martian environments. Furthermore, Martian near- or
subsurface oxychlorine brines, and brines found in potential lifeforms, could
provide a unique niche for biomolecular evolution.
Continuum emission from within the plunging region of black hole discsSérgio Sacani
The thermal continuum emission observed from accreting black holes across X-ray bands has the potential to be leveraged as a
powerful probe of the mass and spin of the central black hole. The vast majority of existing ‘continuum fitting’ models neglect
emission sourced at and within the innermost stable circular orbit (ISCO) of the black hole. Numerical simulations, however,
find non-zero emission sourced from these regions. In this work, we extend existing techniques by including the emission
sourced from within the plunging region, utilizing new analytical models that reproduce the properties of numerical accretion
simulations. We show that in general the neglected intra-ISCO emission produces a hot-and-small quasi-blackbody component,
but can also produce a weak power-law tail for more extreme parameter regions. A similar hot-and-small blackbody component
has been added in by hand in an ad hoc manner to previous analyses of X-ray binary spectra. We show that the X-ray spectrum
of MAXI J1820+070 in a soft-state outburst is extremely well described by a full Kerr black hole disc, while conventional
models that neglect intra-ISCO emission are unable to reproduce the data. We believe this represents the first robust detection of
intra-ISCO emission in the literature, and allows additional constraints to be placed on the MAXI J1820 + 070 black hole spin
which must be low a• < 0.5 to allow a detectable intra-ISCO region. Emission from within the ISCO is the dominant emission
component in the MAXI J1820 + 070 spectrum between 6 and 10 keV, highlighting the necessity of including this region. Our
continuum fitting model is made publicly available.
Have you ever been confused by the myriad of choices offered by AWS for hosting a website or an API?
Lambda, Elastic Beanstalk, Lightsail, Amplify, S3 (and more!) can each host websites + APIs. But which one should we choose?
Which one is cheapest? Which one is fastest? Which one will scale to meet our needs?
Join me in this session as we dive into each AWS hosting service to determine which one is best for your scenario and explain why!
Generating privacy-protected synthetic data using Secludy and MilvusZilliz
During this demo, the founders of Secludy will demonstrate how their system utilizes Milvus to store and manipulate embeddings for generating privacy-protected synthetic data. Their approach not only maintains the confidentiality of the original data but also enhances the utility and scalability of LLMs under privacy constraints. Attendees, including machine learning engineers, data scientists, and data managers, will witness first-hand how Secludy's integration with Milvus empowers organizations to harness the power of LLMs securely and efficiently.
Things to Consider When Choosing a Website Developer for your Website | FODUUFODUU
Choosing the right website developer is crucial for your business. This article covers essential factors to consider, including experience, portfolio, technical skills, communication, pricing, reputation & reviews, cost and budget considerations and post-launch support. Make an informed decision to ensure your website meets your business goals.
Your One-Stop Shop for Python Success: Top 10 US Python Development Providersakankshawande
Simplify your search for a reliable Python development partner! This list presents the top 10 trusted US providers offering comprehensive Python development services, ensuring your project's success from conception to completion.
Climate Impact of Software Testing at Nordic Testing DaysKari Kakkonen
My slides at Nordic Testing Days 6.6.2024
Climate impact / sustainability of software testing discussed on the talk. ICT and testing must carry their part of global responsibility to help with the climat warming. We can minimize the carbon footprint but we can also have a carbon handprint, a positive impact on the climate. Quality characteristics can be added with sustainability, and then measured continuously. Test environments can be used less, and in smaller scale and on demand. Test techniques can be used in optimizing or minimizing number of tests. Test automation can be used to speed up testing.
Unlocking Productivity: Leveraging the Potential of Copilot in Microsoft 365, a presentation by Christoforos Vlachos, Senior Solutions Manager – Modern Workplace, Uni Systems
Fueling AI with Great Data with Airbyte WebinarZilliz
This talk will focus on how to collect data from a variety of sources, leveraging this data for RAG and other GenAI use cases, and finally charting your course to productionalization.
CAKE: Sharing Slices of Confidential Data on BlockchainClaudio Di Ciccio
Presented at the CAiSE 2024 Forum, Intelligent Information Systems, June 6th, Limassol, Cyprus.
Synopsis: Cooperative information systems typically involve various entities in a collaborative process within a distributed environment. Blockchain technology offers a mechanism for automating such processes, even when only partial trust exists among participants. The data stored on the blockchain is replicated across all nodes in the network, ensuring accessibility to all participants. While this aspect facilitates traceability, integrity, and persistence, it poses challenges for adopting public blockchains in enterprise settings due to confidentiality issues. In this paper, we present a software tool named Control Access via Key Encryption (CAKE), designed to ensure data confidentiality in scenarios involving public blockchains. After outlining its core components and functionalities, we showcase the application of CAKE in the context of a real-world cyber-security project within the logistics domain.
Paper: https://doi.org/10.1007/978-3-031-61000-4_16
Cosa hanno in comune un mattoncino Lego e la backdoor XZ?Speck&Tech
ABSTRACT: A prima vista, un mattoncino Lego e la backdoor XZ potrebbero avere in comune il fatto di essere entrambi blocchi di costruzione, o dipendenze di progetti creativi e software. La realtà è che un mattoncino Lego e il caso della backdoor XZ hanno molto di più di tutto ciò in comune.
Partecipate alla presentazione per immergervi in una storia di interoperabilità, standard e formati aperti, per poi discutere del ruolo importante che i contributori hanno in una comunità open source sostenibile.
BIO: Sostenitrice del software libero e dei formati standard e aperti. È stata un membro attivo dei progetti Fedora e openSUSE e ha co-fondato l'Associazione LibreItalia dove è stata coinvolta in diversi eventi, migrazioni e formazione relativi a LibreOffice. In precedenza ha lavorato a migrazioni e corsi di formazione su LibreOffice per diverse amministrazioni pubbliche e privati. Da gennaio 2020 lavora in SUSE come Software Release Engineer per Uyuni e SUSE Manager e quando non segue la sua passione per i computer e per Geeko coltiva la sua curiosità per l'astronomia (da cui deriva il suo nickname deneb_alpha).
GraphRAG for Life Science to increase LLM accuracyTomaz Bratanic
GraphRAG for life science domain, where you retriever information from biomedical knowledge graphs using LLMs to increase the accuracy and performance of generated answers
Taking AI to the Next Level in Manufacturing.pdfssuserfac0301
Read Taking AI to the Next Level in Manufacturing to gain insights on AI adoption in the manufacturing industry, such as:
1. How quickly AI is being implemented in manufacturing.
2. Which barriers stand in the way of AI adoption.
3. How data quality and governance form the backbone of AI.
4. Organizational processes and structures that may inhibit effective AI adoption.
6. Ideas and approaches to help build your organization's AI strategy.
TrustArc Webinar - 2024 Global Privacy SurveyTrustArc
How does your privacy program stack up against your peers? What challenges are privacy teams tackling and prioritizing in 2024?
In the fifth annual Global Privacy Benchmarks Survey, we asked over 1,800 global privacy professionals and business executives to share their perspectives on the current state of privacy inside and outside of their organizations. This year’s report focused on emerging areas of importance for privacy and compliance professionals, including considerations and implications of Artificial Intelligence (AI) technologies, building brand trust, and different approaches for achieving higher privacy competence scores.
See how organizational priorities and strategic approaches to data security and privacy are evolving around the globe.
This webinar will review:
- The top 10 privacy insights from the fifth annual Global Privacy Benchmarks Survey
- The top challenges for privacy leaders, practitioners, and organizations in 2024
- Key themes to consider in developing and maintaining your privacy program
In the rapidly evolving landscape of technologies, XML continues to play a vital role in structuring, storing, and transporting data across diverse systems. The recent advancements in artificial intelligence (AI) present new methodologies for enhancing XML development workflows, introducing efficiency, automation, and intelligent capabilities. This presentation will outline the scope and perspective of utilizing AI in XML development. The potential benefits and the possible pitfalls will be highlighted, providing a balanced view of the subject.
We will explore the capabilities of AI in understanding XML markup languages and autonomously creating structured XML content. Additionally, we will examine the capacity of AI to enrich plain text with appropriate XML markup. Practical examples and methodological guidelines will be provided to elucidate how AI can be effectively prompted to interpret and generate accurate XML markup.
Further emphasis will be placed on the role of AI in developing XSLT, or schemas such as XSD and Schematron. We will address the techniques and strategies adopted to create prompts for generating code, explaining code, or refactoring the code, and the results achieved.
The discussion will extend to how AI can be used to transform XML content. In particular, the focus will be on the use of AI XPath extension functions in XSLT, Schematron, Schematron Quick Fixes, or for XML content refactoring.
The presentation aims to deliver a comprehensive overview of AI usage in XML development, providing attendees with the necessary knowledge to make informed decisions. Whether you’re at the early stages of adopting AI or considering integrating it in advanced XML development, this presentation will cover all levels of expertise.
By highlighting the potential advantages and challenges of integrating AI with XML development tools and languages, the presentation seeks to inspire thoughtful conversation around the future of XML development. We’ll not only delve into the technical aspects of AI-powered XML development but also discuss practical implications and possible future directions.
Ocean lotus Threat actors project by John Sitima 2024 (1).pptxSitimaJohn
Ocean Lotus cyber threat actors represent a sophisticated, persistent, and politically motivated group that poses a significant risk to organizations and individuals in the Southeast Asian region. Their continuous evolution and adaptability underscore the need for robust cybersecurity measures and international cooperation to identify and mitigate the threats posed by such advanced persistent threat groups.
Driving Business Innovation: Latest Generative AI Advancements & Success StorySafe Software
Are you ready to revolutionize how you handle data? Join us for a webinar where we’ll bring you up to speed with the latest advancements in Generative AI technology and discover how leveraging FME with tools from giants like Google Gemini, Amazon, and Microsoft OpenAI can supercharge your workflow efficiency.
During the hour, we’ll take you through:
Guest Speaker Segment with Hannah Barrington: Dive into the world of dynamic real estate marketing with Hannah, the Marketing Manager at Workspace Group. Hear firsthand how their team generates engaging descriptions for thousands of office units by integrating diverse data sources—from PDF floorplans to web pages—using FME transformers, like OpenAIVisionConnector and AnthropicVisionConnector. This use case will show you how GenAI can streamline content creation for marketing across the board.
Ollama Use Case: Learn how Scenario Specialist Dmitri Bagh has utilized Ollama within FME to input data, create custom models, and enhance security protocols. This segment will include demos to illustrate the full capabilities of FME in AI-driven processes.
Custom AI Models: Discover how to leverage FME to build personalized AI models using your data. Whether it’s populating a model with local data for added security or integrating public AI tools, find out how FME facilitates a versatile and secure approach to AI.
We’ll wrap up with a live Q&A session where you can engage with our experts on your specific use cases, and learn more about optimizing your data workflows with AI.
This webinar is ideal for professionals seeking to harness the power of AI within their data management systems while ensuring high levels of customization and security. Whether you're a novice or an expert, gain actionable insights and strategies to elevate your data processes. Join us to see how FME and AI can revolutionize how you work with data!
AI 101: An Introduction to the Basics and Impact of Artificial IntelligenceIndexBug
Imagine a world where machines not only perform tasks but also learn, adapt, and make decisions. This is the promise of Artificial Intelligence (AI), a technology that's not just enhancing our lives but revolutionizing entire industries.