This document provides an overview of an academic presentation on interstellar flight given by Kelvin F. Long, the executive director of the Institute for Interstellar Studies. The presentation discusses the history of interstellar studies and proposals, including projects by the British Interplanetary Society. It also examines the fundamental requirements and challenges of interstellar travel such as the large amounts of energy needed and long mission times. Finally, it introduces the Institute for Interstellar Studies and its mission to promote education and technologies that could enable interstellar spacecraft.
The document provides information about the Sun and planets in our solar system. It states that the Sun is a yellow dwarf star composed primarily of hydrogen that generates energy through nuclear fusion. It accounts for 99.9% of the mass in the solar system. The temperature at the Sun's core is 15 million degrees Celsius. The document also provides brief descriptions of the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and dwarf planet Pluto.
Astronomy - State of the Art - Life in the UniverseChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the potential for life in the universe is covered, including extreme life on Earth, the Drake equation and SETI
This document discusses various concepts and technologies related to interstellar travel, including:
1) Current rocket technologies are insufficient to reach other stars due to limitations of chemical fuels; multistage rockets and new fuels like nuclear or antimatter could help.
2) The nearest star is over 4 light years away, so travel at current speeds would take tens of thousands of years; new propulsion methods like ion drives, solar sails, and ramjets could enable much faster travel.
3) However, special relativity shows that nothing can travel faster than light speed, posing a fundamental limit to interstellar travel; speculative ideas like wormholes or generation ships may be needed to overcome this.
The document proposes a new concept called the New Worlds Imager (NWI) as an alternative to the Terrestrial Planet Finder (TPF) for directly imaging exoplanets. The NWI would use a large starshade and interferometer in space to block starlight and combine light from exoplanets to image them with resolutions of 100km at 10 parsecs. It could directly image biomarkers on Earth-like exoplanets within the next 10-20 years using existing technology and would further the goal of finding life outside our solar system.
Advanced space propulsion concepts for interstellar travelMarcus 2012
When a particle and its antiparticle collide, they annihilate each other and are converted to energy according to Einstein's mass-energy equivalence formula E=mc2. Three concepts for utilizing this are:
1) Magnetic confinement fusion uses magnetic fields to contain a plasma and fuse atomic nuclei for propulsion.
2) Gas-core nuclear fission contains fission fuel in a high-temperature plasma for propulsion, but magnetic containment is challenging.
3) Matter-antimatter annihilation could provide the highest energy density, but generating and containing significant amounts of antimatter poses major technical hurdles.
Astronomy - Stat eof the Art - CosmologyChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the properties of the whole universe are covered, including Hubble expansion, the age and size, the big bang, and dark energy.
Active galaxies can be categorized into three main types: Seyfert galaxies, radio galaxies, and quasars. Seyfert galaxies are active spiral galaxies with non-stellar spectra. Radio galaxies are active elliptical galaxies that also have non-stellar spectra and are strong radio emitters. Quasars are the most luminous active galaxies known, far brighter than normal galaxies, with non-stellar spectra. Centaurus A is the closest active galaxy and provides a unique laboratory for studying these powerful objects, showing evidence of a past merger that fuels activity at its center.
The document provides information about the Sun and planets in our solar system. It states that the Sun is a yellow dwarf star composed primarily of hydrogen that generates energy through nuclear fusion. It accounts for 99.9% of the mass in the solar system. The temperature at the Sun's core is 15 million degrees Celsius. The document also provides brief descriptions of the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and dwarf planet Pluto.
Astronomy - State of the Art - Life in the UniverseChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the potential for life in the universe is covered, including extreme life on Earth, the Drake equation and SETI
This document discusses various concepts and technologies related to interstellar travel, including:
1) Current rocket technologies are insufficient to reach other stars due to limitations of chemical fuels; multistage rockets and new fuels like nuclear or antimatter could help.
2) The nearest star is over 4 light years away, so travel at current speeds would take tens of thousands of years; new propulsion methods like ion drives, solar sails, and ramjets could enable much faster travel.
3) However, special relativity shows that nothing can travel faster than light speed, posing a fundamental limit to interstellar travel; speculative ideas like wormholes or generation ships may be needed to overcome this.
The document proposes a new concept called the New Worlds Imager (NWI) as an alternative to the Terrestrial Planet Finder (TPF) for directly imaging exoplanets. The NWI would use a large starshade and interferometer in space to block starlight and combine light from exoplanets to image them with resolutions of 100km at 10 parsecs. It could directly image biomarkers on Earth-like exoplanets within the next 10-20 years using existing technology and would further the goal of finding life outside our solar system.
Advanced space propulsion concepts for interstellar travelMarcus 2012
When a particle and its antiparticle collide, they annihilate each other and are converted to energy according to Einstein's mass-energy equivalence formula E=mc2. Three concepts for utilizing this are:
1) Magnetic confinement fusion uses magnetic fields to contain a plasma and fuse atomic nuclei for propulsion.
2) Gas-core nuclear fission contains fission fuel in a high-temperature plasma for propulsion, but magnetic containment is challenging.
3) Matter-antimatter annihilation could provide the highest energy density, but generating and containing significant amounts of antimatter poses major technical hurdles.
Astronomy - Stat eof the Art - CosmologyChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the properties of the whole universe are covered, including Hubble expansion, the age and size, the big bang, and dark energy.
Active galaxies can be categorized into three main types: Seyfert galaxies, radio galaxies, and quasars. Seyfert galaxies are active spiral galaxies with non-stellar spectra. Radio galaxies are active elliptical galaxies that also have non-stellar spectra and are strong radio emitters. Quasars are the most luminous active galaxies known, far brighter than normal galaxies, with non-stellar spectra. Centaurus A is the closest active galaxy and provides a unique laboratory for studying these powerful objects, showing evidence of a past merger that fuels activity at its center.
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.
Telescopes allow astronomers to observe the universe in different wavelengths of light. Ground-based telescopes are limited by Earth's atmosphere, so many telescopes have been placed in space. There are two main types of telescopes - refracting telescopes which use lenses and reflecting telescopes which use mirrors. Multiple telescopes can work together using interferometry to achieve the resolution of a larger single telescope. Astronomers use telescopes to take images of celestial objects, perform spectroscopy to analyze light, and monitor changes over time.
Ok, we found a new Earth nearby. Next question is: how do we get there?
The amazing challenge to get mankind to become an interstellar species and how we could potentially get there.
The different technologies involved and the key challenges to overcome.
Welcome to teh next chapter of mankind.
Gamma rays have the shortest wavelengths and highest energy of all electromagnetic waves. They are produced by radioactive decay, nuclear explosions, and extremely hot astronomical objects like supernovae. Gamma rays can penetrate the Earth's atmosphere so astronomers use high-altitude balloons and satellites to observe them. Gamma rays reveal information about violent cosmic events and locations with strong gravitational and magnetic fields like neutron stars and black holes.
The document discusses theoretical solutions for interstellar travel. It outlines three potential propulsion systems: fusion drives, solar sails, and warp drives. Fusion drives use nuclear fusion as propulsion and could reach speeds up to 20% of light, but require advances in fusion technology. Solar sails use radiation pressure for propulsion and existing technology, but would need powerful lasers to reach high speeds. Warp drives theoretically allow faster than light travel by warping space-time, but would require exotic fuels like negative mass. Further research in areas like fusion and detecting negative mass/energy could help develop these technologies to enable humanity to explore beyond the solar system within a human lifetime.
Space telescopes (2/3) - NASA's Active Orbiting SatellitesSteven Belaire
The second of a 3 part series exploring currently active space telescopes. This installment covers NASA's active orbiting satellites (excluding solar telescopes).
This document presents theoretical models for reactionless propulsion and an Earth gravity generator. It discusses inertial and non-inertial frames of reference and how the laws of physics vary between them. The reactionless propulsion model uses a pendulum within a rotating reference frame, where the centrifugal force vectors could potentially cancel out. Calculations determine the system energy and centrifugal forces for different parameters. The Earth gravity generator model places a bob on a spinning axis, where the centrifugal force counteracts gravity at a specific equilibrium RPM.
The document provides information on astrophysics, astronomy, the universe, galaxies, the Sun, and the layers and components of the Sun. It discusses the history of astronomy and how our understanding has developed since the mid-1800s. It also summarizes the history of the Indian Institute of Astrophysics and the 6-inch telescope located there. The 6-inch telescope's components and how it is used to focus images of sunspots are described.
The more we know about the Cosmos the stranger it seems to get. The new Kepler space telescope has detected many new “exoplanet”—planets in other star systems. Some of these planets are quite strange. One has the density of Styrofoam. Another seems to be hotter than the star it revolves around. Kinks in the Kepler telescope’s sensors have been worked around using computers and the ground and it is now providing amazing data from millions of star systems. The refurbished Hubble Space Telescope has now peered more deeply into the past than ever before to almost the dawn of the Universe. In addition, the James Webb Telescope will soon allow us to see even further back in time. Come hear Dr. Eric P. Smith, NASA astrophysicist show and tell us about the Latest and Greatest News from the Cosmos.
The document provides an overview of lessons covering physics topics related to astronomy. It outlines 24 lessons that will cover telescopes, lenses, different types of telescopes, stars, the sun, moon and earth, eclipses, star distances, galaxies, and more. Each lesson includes objectives, literacy and numeracy focuses, and extension questions.
Three astronauts - Neil Armstrong, Michael Collins, and Buzz Aldrin - launched aboard the Apollo 11 spacecraft on a mission to land on the Moon in July 1969. The 8-day mission was successful, with Armstrong and Aldrin becoming the first humans to walk on the lunar surface. However, some conspiracy theorists argue that the Moon landings were faked and did not actually occur. The document then presents several of the most common arguments made by conspiracy theorists claiming to prove the landings were hoaxed, such as the lack of stars or impact craters in photos, unusual shadows, and mysterious reflections. NASA has provided counterarguments for each of these claims based on scientific explanations.
The document summarizes the prospect of UV observations from the Moon using a proposed UV telescope called LUCI. Some key points:
1. LUCI would be a small UV telescope (30cm aperture) to be deployed on the lunar surface by Team Indus, to take advantage of the Moon's stable environment for UV astronomy.
2. The telescope would image bright UV sources like stars and nebulae to magnitudes of 12 to study transients and variability. It would cover 60 square degrees in a lunar day.
3. The design and calibration of LUCI's optics, structure, detectors, and electronics are described, showing it can meet weight and size constraints for deployment on the lunar lander while achieving the
Galaxy Forum USA 2016 - Prof Imke de Pater, UC BerkeleyILOAHawaii
Background:
Galaxy Forum is the primary education and outreach initiative of ILOA, it is an architecture designed to advance 21st Century science, education, enterprise and development around the world.
Galaxy Forums are public events specifically geared towards high school teachers, educators, astronomers of all kinds, students and the general public. Presentations are provided by experts in the fields of astrophysics / galaxy research, space exploration and STEM education, as well as related aspects of culture and traditional knowledge. Interactive panel discussions allow for community participation and integration of local perspectives.
Stats:
Almost 70 Galaxy Forums, with a total of about 300 presentations to date.
Held in 26 locations worldwide including Hawaii, Silicon Valley, Canada, China, India, Southeast Asia, Japan, Europe, Africa, Chile, Brazil, Kansas and New York.
Started with Galaxy Forum USA, July 4, 2008 in Silicon Valley, California.
International Lunar Observatory Association (ILOA) is an interglobal enterprise incorporated in Hawaii as a 501(c)(3) non-profit to expand human knowledge of the Cosmos through observation from our Moon and to participate in internationally cooperative lunar base build-out, with Aloha – the spirit of Hawai`i.
This document outlines a physics lesson plan on telescopes over 24 lessons. It will cover the different types of telescopes like refracting, reflecting, and radio telescopes. It will discuss how telescopes produce images using electromagnetic radiation of different frequencies. Key topics include lenses, star distances, galaxies, and the composition of stars. Lessons will include activities, literacy and numeracy focus, and questions for extension.
Astronomy- State of the art is a course covering the hottest topics in astronomy. In this section, the exotic end states of stars are discussed, including pulsars, neutron stars, and black holes.
Space debris in low-Earth orbit poses a serious and growing threat. There are over 22,000 pieces of debris larger than 10 cm currently orbiting Earth, traveling at speeds sufficient to damage satellites. If left unchecked, the amount of debris will continue to grow exponentially through collisions in a process known as the Kessler Syndrome, which could render space exploration and satellite use impossible for generations. Solutions require both mitigation efforts to limit further debris creation as well as active removal of existing debris through methods like lasers, electromagnets, or debris-capturing space structures. International cooperation will be needed to implement solutions and avoid a space debris disaster.
This document discusses dark matter detection. It presents evidence for the existence of dark matter from observations of galaxy clusters, and notes that dark matter is thought to make up around a quarter of the universe. It also mentions an alternative theory that dark matter may not exist and that modified gravity could explain observations instead. The document outlines different approaches to detecting dark matter, including looking for it at different astronomical scales and using multi-wavelength, multi-epoch, and multi-messenger observations.
September 2015, the LIGO detectors in the USA saw space vibrate with gravitational waves for the very first time. Although the signal was extremely weak when it reached Earth, it is already promising a revolution in astrophysics.
The document discusses the distance ladder, which is an attempt to determine astronomical distances by using a series of methods that build on one another. Within the Solar System, distances are measured using radar ranging. Within the galaxy, distances are measured using stellar parallax, main sequence fitting, and properties of Cepheid variable stars. Further out in the universe, distances are measured using the Tully-Fisher relation, Type Ia supernovae, brightest cluster galaxies, and Hubble's law. The document aims to answer fundamental questions about what exists in the universe and how large it is.
The document discusses neutron stars and pulsars. It begins by outlining predictions about neutron stars, including their small radius of 10-80 km but large mass over 1.4 times the sun's mass. It then explains how conservation of angular momentum causes neutron stars to spin rapidly as the core collapses. The discovery of pulsars is summarized, including how their periodic emission can be explained by a rotating misaligned magnetic field. The document concludes by briefly introducing black holes and relating them to Einstein's theory of general relativity.
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.
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.
Telescopes allow astronomers to observe the universe in different wavelengths of light. Ground-based telescopes are limited by Earth's atmosphere, so many telescopes have been placed in space. There are two main types of telescopes - refracting telescopes which use lenses and reflecting telescopes which use mirrors. Multiple telescopes can work together using interferometry to achieve the resolution of a larger single telescope. Astronomers use telescopes to take images of celestial objects, perform spectroscopy to analyze light, and monitor changes over time.
Ok, we found a new Earth nearby. Next question is: how do we get there?
The amazing challenge to get mankind to become an interstellar species and how we could potentially get there.
The different technologies involved and the key challenges to overcome.
Welcome to teh next chapter of mankind.
Gamma rays have the shortest wavelengths and highest energy of all electromagnetic waves. They are produced by radioactive decay, nuclear explosions, and extremely hot astronomical objects like supernovae. Gamma rays can penetrate the Earth's atmosphere so astronomers use high-altitude balloons and satellites to observe them. Gamma rays reveal information about violent cosmic events and locations with strong gravitational and magnetic fields like neutron stars and black holes.
The document discusses theoretical solutions for interstellar travel. It outlines three potential propulsion systems: fusion drives, solar sails, and warp drives. Fusion drives use nuclear fusion as propulsion and could reach speeds up to 20% of light, but require advances in fusion technology. Solar sails use radiation pressure for propulsion and existing technology, but would need powerful lasers to reach high speeds. Warp drives theoretically allow faster than light travel by warping space-time, but would require exotic fuels like negative mass. Further research in areas like fusion and detecting negative mass/energy could help develop these technologies to enable humanity to explore beyond the solar system within a human lifetime.
Space telescopes (2/3) - NASA's Active Orbiting SatellitesSteven Belaire
The second of a 3 part series exploring currently active space telescopes. This installment covers NASA's active orbiting satellites (excluding solar telescopes).
This document presents theoretical models for reactionless propulsion and an Earth gravity generator. It discusses inertial and non-inertial frames of reference and how the laws of physics vary between them. The reactionless propulsion model uses a pendulum within a rotating reference frame, where the centrifugal force vectors could potentially cancel out. Calculations determine the system energy and centrifugal forces for different parameters. The Earth gravity generator model places a bob on a spinning axis, where the centrifugal force counteracts gravity at a specific equilibrium RPM.
The document provides information on astrophysics, astronomy, the universe, galaxies, the Sun, and the layers and components of the Sun. It discusses the history of astronomy and how our understanding has developed since the mid-1800s. It also summarizes the history of the Indian Institute of Astrophysics and the 6-inch telescope located there. The 6-inch telescope's components and how it is used to focus images of sunspots are described.
The more we know about the Cosmos the stranger it seems to get. The new Kepler space telescope has detected many new “exoplanet”—planets in other star systems. Some of these planets are quite strange. One has the density of Styrofoam. Another seems to be hotter than the star it revolves around. Kinks in the Kepler telescope’s sensors have been worked around using computers and the ground and it is now providing amazing data from millions of star systems. The refurbished Hubble Space Telescope has now peered more deeply into the past than ever before to almost the dawn of the Universe. In addition, the James Webb Telescope will soon allow us to see even further back in time. Come hear Dr. Eric P. Smith, NASA astrophysicist show and tell us about the Latest and Greatest News from the Cosmos.
The document provides an overview of lessons covering physics topics related to astronomy. It outlines 24 lessons that will cover telescopes, lenses, different types of telescopes, stars, the sun, moon and earth, eclipses, star distances, galaxies, and more. Each lesson includes objectives, literacy and numeracy focuses, and extension questions.
Three astronauts - Neil Armstrong, Michael Collins, and Buzz Aldrin - launched aboard the Apollo 11 spacecraft on a mission to land on the Moon in July 1969. The 8-day mission was successful, with Armstrong and Aldrin becoming the first humans to walk on the lunar surface. However, some conspiracy theorists argue that the Moon landings were faked and did not actually occur. The document then presents several of the most common arguments made by conspiracy theorists claiming to prove the landings were hoaxed, such as the lack of stars or impact craters in photos, unusual shadows, and mysterious reflections. NASA has provided counterarguments for each of these claims based on scientific explanations.
The document summarizes the prospect of UV observations from the Moon using a proposed UV telescope called LUCI. Some key points:
1. LUCI would be a small UV telescope (30cm aperture) to be deployed on the lunar surface by Team Indus, to take advantage of the Moon's stable environment for UV astronomy.
2. The telescope would image bright UV sources like stars and nebulae to magnitudes of 12 to study transients and variability. It would cover 60 square degrees in a lunar day.
3. The design and calibration of LUCI's optics, structure, detectors, and electronics are described, showing it can meet weight and size constraints for deployment on the lunar lander while achieving the
Galaxy Forum USA 2016 - Prof Imke de Pater, UC BerkeleyILOAHawaii
Background:
Galaxy Forum is the primary education and outreach initiative of ILOA, it is an architecture designed to advance 21st Century science, education, enterprise and development around the world.
Galaxy Forums are public events specifically geared towards high school teachers, educators, astronomers of all kinds, students and the general public. Presentations are provided by experts in the fields of astrophysics / galaxy research, space exploration and STEM education, as well as related aspects of culture and traditional knowledge. Interactive panel discussions allow for community participation and integration of local perspectives.
Stats:
Almost 70 Galaxy Forums, with a total of about 300 presentations to date.
Held in 26 locations worldwide including Hawaii, Silicon Valley, Canada, China, India, Southeast Asia, Japan, Europe, Africa, Chile, Brazil, Kansas and New York.
Started with Galaxy Forum USA, July 4, 2008 in Silicon Valley, California.
International Lunar Observatory Association (ILOA) is an interglobal enterprise incorporated in Hawaii as a 501(c)(3) non-profit to expand human knowledge of the Cosmos through observation from our Moon and to participate in internationally cooperative lunar base build-out, with Aloha – the spirit of Hawai`i.
This document outlines a physics lesson plan on telescopes over 24 lessons. It will cover the different types of telescopes like refracting, reflecting, and radio telescopes. It will discuss how telescopes produce images using electromagnetic radiation of different frequencies. Key topics include lenses, star distances, galaxies, and the composition of stars. Lessons will include activities, literacy and numeracy focus, and questions for extension.
Astronomy- State of the art is a course covering the hottest topics in astronomy. In this section, the exotic end states of stars are discussed, including pulsars, neutron stars, and black holes.
Space debris in low-Earth orbit poses a serious and growing threat. There are over 22,000 pieces of debris larger than 10 cm currently orbiting Earth, traveling at speeds sufficient to damage satellites. If left unchecked, the amount of debris will continue to grow exponentially through collisions in a process known as the Kessler Syndrome, which could render space exploration and satellite use impossible for generations. Solutions require both mitigation efforts to limit further debris creation as well as active removal of existing debris through methods like lasers, electromagnets, or debris-capturing space structures. International cooperation will be needed to implement solutions and avoid a space debris disaster.
This document discusses dark matter detection. It presents evidence for the existence of dark matter from observations of galaxy clusters, and notes that dark matter is thought to make up around a quarter of the universe. It also mentions an alternative theory that dark matter may not exist and that modified gravity could explain observations instead. The document outlines different approaches to detecting dark matter, including looking for it at different astronomical scales and using multi-wavelength, multi-epoch, and multi-messenger observations.
September 2015, the LIGO detectors in the USA saw space vibrate with gravitational waves for the very first time. Although the signal was extremely weak when it reached Earth, it is already promising a revolution in astrophysics.
The document discusses the distance ladder, which is an attempt to determine astronomical distances by using a series of methods that build on one another. Within the Solar System, distances are measured using radar ranging. Within the galaxy, distances are measured using stellar parallax, main sequence fitting, and properties of Cepheid variable stars. Further out in the universe, distances are measured using the Tully-Fisher relation, Type Ia supernovae, brightest cluster galaxies, and Hubble's law. The document aims to answer fundamental questions about what exists in the universe and how large it is.
The document discusses neutron stars and pulsars. It begins by outlining predictions about neutron stars, including their small radius of 10-80 km but large mass over 1.4 times the sun's mass. It then explains how conservation of angular momentum causes neutron stars to spin rapidly as the core collapses. The discovery of pulsars is summarized, including how their periodic emission can be explained by a rotating misaligned magnetic field. The document concludes by briefly introducing black holes and relating them to Einstein's theory of general relativity.
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.
The document discusses near-Earth objects such as asteroids and comets that pose a potential hazard to Earth, noting that over 8,000 near-Earth objects have been discovered so far, including over 1,200 that are considered potentially hazardous asteroids due to their close orbital approaches to Earth. It also provides background on the composition, origins, and properties of asteroids, comets, meteoroids and related small solar system bodies.
This document provides an overview of human understanding of the universe over the past 3000 years. It begins with ancient Greek philosophers' early concepts of astronomy and the structure of the universe. It then discusses the major scientific breakthroughs from the 15th century onward that led to modern cosmological theories, including the work of Copernicus, Kepler, Galileo, Newton, Maxwell, Einstein and others. The document concludes by noting some of the key discoveries of the early 20th century that helped establish modern physics and our current understanding of the universe.
Presentation Evidence for the Big Bang_p.pptLakdjhdjsak
Three key pieces of evidence support the Big Bang theory of the origin and evolution of the universe:
1. The expansion of the universe, as evidenced by the redshifting of light from distant galaxies and interpreted by Hubble's law.
2. The abundance of hydrogen and helium matches what would be predicted from nucleosynthesis in the early universe.
3. The discovery of cosmic microwave background radiation, which has properties matching predictions from the Big Bang theory.
Astronomy - State of the Art - GalaxiesChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the properties of galaxies are discussed, including supermassive black holes and dark matter.
This document provides information about space, cosmology, the Big Bang theory, and the formation and significance of stars. It discusses what space is, the study of cosmology, evidence for the Big Bang, how stars are formed from nebulae and gravitational collapse, and how stars provide light, heat, energy and are essential for life on Earth.
IB Astrophysics - cosmology - Flippingphysics by nothingnerdyNothingnerdy
The document summarizes key concepts in cosmology, including Olbers' paradox, the expanding universe, the Big Bang theory, and evidence like the cosmic microwave background radiation. It discusses how the universe originated approximately 13.7 billion years ago in a massive expansion from a single point. The universe is still expanding today, and its fate depends on whether it has a flat, closed, or open geometry based on its total mass density. While most mass is dark matter and dark energy, their exact nature remains unknown. International space projects seek to further understand these cosmological questions through observation and research.
Space weather and potential impact on earth’s climate dec 19 10 v2Poramate Minsiri
This document discusses space weather and its potential impacts on Earth's climate and seismic activity. It provides an overview of the solar system and its dynamics, as well as how our solar system interacts with the Milky Way galaxy and larger universe. Recent observations have found evidence that the outer boundaries of our solar system are being compressed as we pass through Galactic clouds, allowing more cosmic rays and energetic particles to enter the inner solar system. This could affect Earth's climate and increase seismic activity. The document also discusses changes observed on other planets in our solar system, such as the growth of dark spots on Pluto and changes in cloud cover on Mars.
ILOA Galaxy Forum Europe 2013 - dark matter in galaxies - dr benoit famaeyILOAHawaii
This document discusses the history and current state of the dark matter problem in astrophysics. It summarizes that observations in the 1930s and 1970s found that galaxies and galaxy clusters contain far more mass than can be accounted for by the visible stars and gas, with the mass increasing farther from galaxy centers. This is known as the "missing mass" problem. The current favored model, called Lambda Cold Dark Matter (Lambda CDM), posits that dark matter makes up 85% of all matter in the universe and helps explain large scale structure formation. However, the nature of dark matter remains unknown, and alternative gravitational theories have not been ruled out. Future experiments aim to directly detect dark matter particles or test gravitational theories on larger scales
Project Icarus is a multi-year volunteer research study backed by the British Interplanetary Society and Icarus Interstellar to design an unmanned fusion-propelled interstellar probe. The goal is to design a probe using current or near-future technology that could deliver scientific data from another star system within 100 years. Previous studies include Project Daedalus from the 1970s, which first studied the challenges of interstellar travel. Project Icarus has evaluated various propulsion methods including fusion rockets, solar and laser sails, and is currently evaluating the "Firefly" design which uses a z-pinch fusion engine. Firefly would use deuterium-deuterium fusion and aims to overcome challenges
Gravitational Wave Astronomy is a fascinating discovery made a few years ago that changed the notions of modern physics. This presentation won the 3rd Prize in the SPIE student chapter's Oral Presetation in my college.
This is a very broad overview of cosmology. It includes an introduction to galaxies, the large scale structure of the universe, black holes, and the fate of the universe. It is intended for teenagers and up.
- The document discusses the asteroid 1986 DA and its potential for asteroid mining. 1986 DA is a 2km metallic M-type near-Earth asteroid located within Earth's orbit.
- Radar observations have found 1986 DA to be highly reflective due to its metallic composition, which is estimated to contain over $1 trillion worth of platinum and other precious metals.
- Mining 1986 DA could involve collecting surface materials or transporting the entire asteroid. It represents a potentially lucrative target for asteroid mining ventures due to its composition and accessible orbit.
This document discusses space technology, both present and future. It defines space as the area above Earth's atmosphere. Present space technology includes the Hubble Space Telescope, Curiosity rover, and Kepler Spacecraft, which have made discoveries about deep space and exoplanets. Future technologies may utilize antimatter, lasers/microwaves from Earth, or solar power to enable more efficient space travel.
1. The document discusses the history and formation of black holes. It explains that black holes were first conceptualized by scientists like Michell, Laplace, Einstein, and Schwarzschild and can form when massive stars collapse at the end of their life.
2. It provides classifications of black holes based on mass and describes their characteristics like intense gravity and density that causes even light to be trapped. Accretion disks and plasma jets are also summarized.
3. Detection methods are summarized, noting that black holes cannot be seen directly but their effects like gravitational lensing and orbits of nearby stars can provide evidence of their existence.
The CONTOUR mission will send a spacecraft to fly within 100 km of the nuclei of at least two comets, Comet Encke in November 2003 and Comet Schwassmann-Wachmann 3 in June 2006, to assess the diversity of comet nuclei and how they have evolved since forming over 4.5 billion years ago. The spacecraft will take high resolution images and map the composition of the nuclei surfaces. It will also analyze the gas and dust surrounding the nuclei to learn about their composition. The spacecraft is designed to withstand speeds particles near the comet nuclei and has solid-state recorders to store the collected data.
ED Cosexx - A SPACE TRAVELLING CORPORATION THAT AIMS TO ACHIEVE INTERGALACTIC...narutorasengan2327
COSEXX is a space technology company aiming to transform space exploration through intergalactic travel. Their main product is the ISTS-2700X spacecraft, which uses a warp drive to travel at nearly 3 million km/hr, 2700 times the speed of light. It can carry 50 people and 700 tons of cargo. COSEXX plans to use the ISTS-2700X to establish sustainable environments on life-supporting planets and expand humanity across galaxies. They aim to raise $1.5 billion to fund initial research and development of the warp drive technology and spacecraft.
- Dark matter is an invisible form of matter that accounts for approximately 27% of the matter in the universe. Its existence and properties are inferred through its gravitational effects such as the motions of visible matter and gravitational lensing. However, the exact nature and composition of dark matter remains unknown.
- Dark energy is thought to be responsible for the accelerating expansion of the universe, accounting for approximately 68% of the total mass-energy content. Its existence helps explain observations that the expansion rate of the universe is accelerating rather than slowing down. However, the exact nature and properties of dark energy are not well understood.
- Future experiments aim to directly detect dark matter particles and gather more precise cosmological data to help distinguish between theories
Similar to Institute for Interstellar Studies (20)
A Business Analysis of a SKYLON Based European Launch Service OperatorA. Rocketeer
The document summarizes a study conducted between 2012-2014 by an industrial consortium for the European Space Agency to explore the feasibility of using Skylon, a single stage reusable launch system, as the basis for a new European launch service operator. The study looked at both a Skylon operator business model and a Skylon manufacturer business model. It found that the only viable approach was an "airline" model where the manufacturer sells Skylons to multiple operators. Under reasonable assumptions, the manufacturer could expect around a 10% return, sufficient to attract public-private funding. The operator business also showed potential for commercial viability even at lower launch prices to match expendable systems.
Tranquility Aerospace Ltd is a privately owned engineering company based in Oxfordshire that offers automation design and manufacturing services to customers like Festo, Intelligent Energy, Ford, Bosch, Parker, Bentley, and Cosworth. The company directors have over 80 years of combined engineering experience. One of Tranquility's projects is Devon One, a single-stage, fully reusable vertical take-off and landing vehicle that can carry a 30-40kg payload to an altitude of 100km and return to its point of origin or another location. Tranquility also conducts research and testing in areas like propulsion, materials, and software.
This document describes a competition to award funding for innovative space propulsion ideas. It provides information on the prizes, submission and judging process. The top prize is £10k for exploratory ideas. Pitches must be 8 minutes and cover the challenge addressed, solution, evidence it will work, and plans for prize money. Judging criteria include relevance, innovation, benefits, and quality of presentation. Rules require submissions by UK entrants by February 20th and presentations on March 18th in London. Intellectual property remains with winners, and funding must be used for continued research.
Reaction Engines has made progress on their Skylon single-stage-to-orbit spaceplane and its SABRE engine. They completed a technology demonstration program for the SABRE engine's pre-cooler system, successfully testing a full-scale pre-cooler module that cooled air to below -100°C for over 5 minutes. Reaction Engines will now begin a £250 million program to demonstrate the engine technologies at a system level and advance the SABRE engine design to critical design review.
The document outlines the UK space sector's achievements and challenges in accelerating space-enabled economic growth. It identifies key markets such as satellite broadband, maritime surveillance, and location-based services that could drive growth. Recommendations include promoting space benefits, increasing exports, stimulating SMEs, and regulating supportively. Implementing identified actions could help triple the upstream space economy and achieve the target of £40 billion in space-enabled turnover by 2030.
IGS Restack Workshop Presentation: Nov 2012A. Rocketeer
The document outlines a vision for the UK space sector in 2030. It discusses establishing a vision to guide growth of the sector and attract political and public support. Some key points include setting objectives to visualize a space-enabled world in 2030 and how the UK can benefit, as well as illustrating benefits of sustained UK leadership in this growing sector. It also reviews progress on recommendations from the 2010 UK Space Innovation and Growth Strategy (IGS) to support the sector.
Future of UK Space Science Missions: Oct 2012A. Rocketeer
The document discusses the future of UK space science missions. It notes that half of UK government space spending is on space science through ESA programs like the Mandatory Science Programme and UK National Programme. Upcoming missions by the end of the decade include Gaia, LISA Pathfinder, BepiColombo, JWST, and the first two Medium-class missions in ESA's Cosmic Vision program. The UK plays a key role in these missions and seeks to maximize returns through coordination with STFC. The dual key mechanism with STFC supports this coordination.
World Space Programs & Prospects: A European PerspectiveA. Rocketeer
This document discusses European space programs and prospects from a European perspective. It summarizes current and future European orbital and suborbital launch systems as well as commercial space companies. It notes that government funding for space programs is unlikely to increase significantly due to budget constraints, but commercial space companies exploiting new technologies and US-developed systems have growth potential. In particular, testing of Reaction Engines' heat exchanger technology is key to financing future development efforts in Europe, and suborbital spaceflight services are expected to see major growth driven by European companies operating reusable launch vehicles developed in the US.
Satellite Applications Catapult Centre OverviewA. Rocketeer
The document proposes establishing a Satellite Applications Catapult Centre to drive innovation in satellite technology and applications. Satellites can provide global communications, broadcasting, positioning and observation. The centre would provide end-to-end capabilities to help ideas commercialize, link existing space companies with new players, and prototype new applications like mobile communications and environmental monitoring to generate economic growth. It recommends establishing the centre to help overcome challenges of commercializing research and industrializing innovations in satellite technologies.
Progress on the SKYLON Reusable SpaceplaneA. Rocketeer
The document provides an update on the progress of Reaction Engines' Skylon reusable spaceplane and SABRE engine programs. It discusses the development of the SABRE engine technology through ground testing, the design of the SABRE4 engine, and compatibility with vehicle requirements. It outlines plans for a flight test of the engine nacelle and estimates costs for demonstrating the engine technology and designing the SABRE4 engine as part of a proposed 30 month Phase 3 program. An independent review by the UK Space Agency and ESA found no critical issues identified for either the Skylon vehicle or SABRE engine programs.
The document discusses the NSTP Space for Growth Competition, which provides funding for collaborative research and development projects with the space sector. It offers two funding streams: Fastrack grants of £50k-£100k for 6-9 month projects, and larger Flagship grants of up to £2m for 1-2 year projects. 54 applications were received for Fastrack grants and 11 for Flagship grants. Strong SME participation was seen, with over half of project leads being SMEs. Projects covered several areas identified in the UK space innovation strategy.
The document discusses the commercial spaceflight revolution and emerging private sector efforts to develop low-cost space technologies. Key points include private companies developing suborbital spacecraft for space tourism, orbital vehicles to resupply the ISS, plans for private space stations, efforts to return to the Moon and mine its resources, and solar power satellites. Private rocket companies like SpaceX are also developing technologies to enable lower-cost access to orbit and beyond.
UKSA National Space Technology StrategyA. Rocketeer
The document presents the National Space Technology Strategy for the UK. It aims to increase the UK's share of the global space economy, which is predicted to grow to £400 billion annually within 20 years. The strategy identifies 5 technology roadmaps and sectors to focus on. It recommends establishing a cross-sector National Space Technology program jointly funded by industry and government, rising to £100 million annually by 2015/16, to develop technologies, increase competitiveness, and create jobs in the growing space sector. The strategy aims to leverage existing UK space capabilities and investments to capture a greater share of global growth opportunities in space technologies and applications.
The document outlines the UK Space Agency's access to space roadmap from 2011-2022. It details both market and technology developments for small satellite launch services, novel low thrust orbits, demonstration of new platform and payload technologies, and development of technologies like Skylon, expandable cubesats, orbit transfer units, small satellite launch boosters, and more. The roadmap outlines increasing the technology readiness levels (TRLs) of these technologies from lower to higher levels between 2011-2022.
NAUTILUS-X Future in Space Operations (FISO) Group PresentationA. Rocketeer
Nautilus-X: A presentation at the Future In Space Operations teleconference on Jan 26th 2011, given by Mark Holderman and Edward Henderson of NASA JSC.
Why You Should Replace Windows 11 with Nitrux Linux 3.5.0 for enhanced perfor...SOFTTECHHUB
The choice of an operating system plays a pivotal role in shaping our computing experience. For decades, Microsoft's Windows has dominated the market, offering a familiar and widely adopted platform for personal and professional use. However, as technological advancements continue to push the boundaries of innovation, alternative operating systems have emerged, challenging the status quo and offering users a fresh perspective on computing.
One such alternative that has garnered significant attention and acclaim is Nitrux Linux 3.5.0, a sleek, powerful, and user-friendly Linux distribution that promises to redefine the way we interact with our devices. With its focus on performance, security, and customization, Nitrux Linux presents a compelling case for those seeking to break free from the constraints of proprietary software and embrace the freedom and flexibility of open-source computing.
Let's Integrate MuleSoft RPA, COMPOSER, APM with AWS IDP along with Slackshyamraj55
Discover the seamless integration of RPA (Robotic Process Automation), COMPOSER, and APM with AWS IDP enhanced with Slack notifications. Explore how these technologies converge to streamline workflows, optimize performance, and ensure secure access, all while leveraging the power of AWS IDP and real-time communication via Slack notifications.
UiPath Test Automation using UiPath Test Suite series, part 6DianaGray10
Welcome to UiPath Test Automation using UiPath Test Suite series part 6. In this session, we will cover Test Automation with generative AI and Open AI.
UiPath Test Automation with generative AI and Open AI webinar offers an in-depth exploration of leveraging cutting-edge technologies for test automation within the UiPath platform. Attendees will delve into the integration of generative AI, a test automation solution, with Open AI advanced natural language processing capabilities.
Throughout the session, participants will discover how this synergy empowers testers to automate repetitive tasks, enhance testing accuracy, and expedite the software testing life cycle. Topics covered include the seamless integration process, practical use cases, and the benefits of harnessing AI-driven automation for UiPath testing initiatives. By attending this webinar, testers, and automation professionals can gain valuable insights into harnessing the power of AI to optimize their test automation workflows within the UiPath ecosystem, ultimately driving efficiency and quality in software development processes.
What will you get from this session?
1. Insights into integrating generative AI.
2. Understanding how this integration enhances test automation within the UiPath platform
3. Practical demonstrations
4. Exploration of real-world use cases illustrating the benefits of AI-driven test automation for UiPath
Topics covered:
What is generative AI
Test Automation with generative AI and Open AI.
UiPath integration with generative AI
Speaker:
Deepak Rai, Automation Practice Lead, Boundaryless Group and UiPath MVP
Communications Mining Series - Zero to Hero - Session 1DianaGray10
This session provides introduction to UiPath Communication Mining, importance and platform overview. You will acquire a good understand of the phases in Communication Mining as we go over the platform with you. Topics covered:
• Communication Mining Overview
• Why is it important?
• How can it help today’s business and the benefits
• Phases in Communication Mining
• Demo on Platform overview
• Q/A
Infrastructure Challenges in Scaling RAG with Custom AI modelsZilliz
Building Retrieval-Augmented Generation (RAG) systems with open-source and custom AI models is a complex task. This talk explores the challenges in productionizing RAG systems, including retrieval performance, response synthesis, and evaluation. We’ll discuss how to leverage open-source models like text embeddings, language models, and custom fine-tuned models to enhance RAG performance. Additionally, we’ll cover how BentoML can help orchestrate and scale these AI components efficiently, ensuring seamless deployment and management of RAG systems in the cloud.
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!
“An Outlook of the Ongoing and Future Relationship between Blockchain Technologies and Process-aware Information Systems.” Invited talk at the joint workshop on Blockchain for Information Systems (BC4IS) and Blockchain for Trusted Data Sharing (B4TDS), co-located with with the 36th International Conference on Advanced Information Systems Engineering (CAiSE), 3 June 2024, Limassol, Cyprus.
Building Production Ready Search Pipelines with Spark and MilvusZilliz
Spark is the widely used ETL tool for processing, indexing and ingesting data to serving stack for search. Milvus is the production-ready open-source vector database. In this talk we will show how to use Spark to process unstructured data to extract vector representations, and push the vectors to Milvus vector database for search serving.
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.
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).
Sudheer Mechineni, Head of Application Frameworks, Standard Chartered Bank
Discover how Standard Chartered Bank harnessed the power of Neo4j to transform complex data access challenges into a dynamic, scalable graph database solution. This keynote will cover their journey from initial adoption to deploying a fully automated, enterprise-grade causal cluster, highlighting key strategies for modelling organisational changes and ensuring robust disaster recovery. Learn how these innovations have not only enhanced Standard Chartered Bank’s data infrastructure but also positioned them as pioneers in the banking sector’s adoption of graph technology.
HCL Notes and Domino License Cost Reduction in the World of DLAUpanagenda
Webinar Recording: https://www.panagenda.com/webinars/hcl-notes-and-domino-license-cost-reduction-in-the-world-of-dlau/
The introduction of DLAU and the CCB & CCX licensing model caused quite a stir in the HCL community. As a Notes and Domino customer, you may have faced challenges with unexpected user counts and license costs. You probably have questions on how this new licensing approach works and how to benefit from it. Most importantly, you likely have budget constraints and want to save money where possible. Don’t worry, we can help with all of this!
We’ll show you how to fix common misconfigurations that cause higher-than-expected user counts, and how to identify accounts which you can deactivate to save money. There are also frequent patterns that can cause unnecessary cost, like using a person document instead of a mail-in for shared mailboxes. We’ll provide examples and solutions for those as well. And naturally we’ll explain the new licensing model.
Join HCL Ambassador Marc Thomas in this webinar with a special guest appearance from Franz Walder. It will give you the tools and know-how to stay on top of what is going on with Domino licensing. You will be able lower your cost through an optimized configuration and keep it low going forward.
These topics will be covered
- Reducing license cost by finding and fixing misconfigurations and superfluous accounts
- How do CCB and CCX licenses really work?
- Understanding the DLAU tool and how to best utilize it
- Tips for common problem areas, like team mailboxes, functional/test users, etc
- Practical examples and best practices to implement right away
Removing Uninteresting Bytes in Software FuzzingAftab Hussain
Imagine a world where software fuzzing, the process of mutating bytes in test seeds to uncover hidden and erroneous program behaviors, becomes faster and more effective. A lot depends on the initial seeds, which can significantly dictate the trajectory of a fuzzing campaign, particularly in terms of how long it takes to uncover interesting behaviour in your code. We introduce DIAR, a technique designed to speedup fuzzing campaigns by pinpointing and eliminating those uninteresting bytes in the seeds. Picture this: instead of wasting valuable resources on meaningless mutations in large, bloated seeds, DIAR removes the unnecessary bytes, streamlining the entire process.
In this work, we equipped AFL, a popular fuzzer, with DIAR and examined two critical Linux libraries -- Libxml's xmllint, a tool for parsing xml documents, and Binutil's readelf, an essential debugging and security analysis command-line tool used to display detailed information about ELF (Executable and Linkable Format). Our preliminary results show that AFL+DIAR does not only discover new paths more quickly but also achieves higher coverage overall. This work thus showcases how starting with lean and optimized seeds can lead to faster, more comprehensive fuzzing campaigns -- and DIAR helps you find such seeds.
- These are slides of the talk given at IEEE International Conference on Software Testing Verification and Validation Workshop, ICSTW 2022.
Dr. Sean Tan, Head of Data Science, Changi Airport Group
Discover how Changi Airport Group (CAG) leverages graph technologies and generative AI to revolutionize their search capabilities. This session delves into the unique search needs of CAG’s diverse passengers and customers, showcasing how graph data structures enhance the accuracy and relevance of AI-generated search results, mitigating the risk of “hallucinations” and improving the overall customer journey.
In his public lecture, Christian Timmerer provides insights into the fascinating history of video streaming, starting from its humble beginnings before YouTube to the groundbreaking technologies that now dominate platforms like Netflix and ORF ON. Timmerer also presents provocative contributions of his own that have significantly influenced the industry. He concludes by looking at future challenges and invites the audience to join in a discussion.
1. Interstellar Flight:
Discovering the Limits of the Possible
Kelvin F. Long
kelvin.long@i4is.org
Executive Director
Institute for Interstellar Studies
Chief Editor, Journal of the British Interplanetary Society
Presented at UKSEDS, University of Bristol,
England, February 2013
2. Contents
• The British
Interplanetary
Society
• Interstellar
Studies
• The Institute for
Interstellar
Studies
2
5. BIS (from imagination to reality)
THE IMAGINATION WALL THE REALITY WALL
BRITISH
INTERPLANETARY
SOCIETY
Ideas (DOMAIN) Industry
Conjecture Academia
Creativity Government
Concepts Inventions
Stories Technologies
Solutions Spin-offs
philosophy careers
SPIN-IN SPIN-OUT
5
6. BIS Projects (Imagination to Reality)
BIS Project Megaroc (1946) NASA Project Mercury-Redstone (1960-61)
6
8. BIS Projects (Imagination to Reality)
J.Verne, “From Earth to the Moon”, 1865 H.G.Wells, “The First Men in the Moon”, 1901
Ross, H.E, “The BIS Space-Ship”1939. NASA Project Apollo (1969)
8
9. BIS Project KickSat
Project KickSat is an initiative of Zac Manchester, Cornell
University, USA and the BIS are launching a fleet of ChipSats or
Sprites into Earth orbit.
RECRUITS NEEDED!!
9
10. BIS Project 2033 (NEW Launch)
What is the state of space exploration in the year 2033?
Are you the next visionary?
Send us your submission RECRUITS NEEDED!!
10
12. BIS Project STARDROP (New Launch)
Solar Thermal Amplified Radiation
Dynamic Relay of Orbiting Power
A project to design a 10 GW Solar Collector station in space capable of
delivering energy to a space habitat at the L5 point.
RECRUITS NEEDED!!
12
16. Motivations
“I can never look now at the Milky Way without wondering from
which of those banked clouds of stars the emissaries are
coming…I do not think we will have to wait for long”.
Arthur C Clarke
Sir Arthur C. Clarke
16
17. The Size of Space and Beyond
• Barred spiral galaxy
• 100-400 billion stars
• Oldest 13.2 billion years
• 1×1012Msun
• 200 million years to rotate
• 27kLY to the centre from the Sun
• 1MLY Diameter
• 1kLY thick
• Even if we could travel at the speed of light,
would take 27,000 years to reach Galactic
centre and would take 1 millions years for
any starship to cross entire galaxy, or 1,000
years to penetrate galactic thickness.
The Milky Way galaxy • Implications for Fermi Paradox: A
statement on the apparent contradiction
between our theoretical expectations for
intelligent life in the Universe and our
observations.
17
18.
19. Voyager 1
• Launched 1977
• Currently at around 120 AU distance
• 1AU = 1.496×1011 m, so Voyager at
1.795×1013m. Light travels at 3×108
m/s, so Voyager at 59,840 s, 997
minutes or 16.62 light hours away.
• Travelling at 17.4 km/s or 3.67
AU/year, which is 0.0058%c.
• So would take 74,138 years to reach
Alpha Centauri if it was pointing that
way.
• Conclusion: We need to go faster and
further.
19
23. Advanced Space Propulsion
• Electric • Fission
• Nuclear Electric • Fission/Fusion
• Laser Thermal • Fusion
• Solar Thermal • External Nuclear Pulse
• Nuclear Thermal • Antimatter Catalysed Fusion
• Plasma Drives • Interstellar Ramjets
• EM Mass Drivers • Negative Energy
• Particle Beamers • Space Drives
• Solar Sails • Warp Drives
• Laser Sails • Worm Holes
• Microwave Beam Sails • Time Machines
The technology readiness maturity distinguishes
between ‘imagination’ and ‘reality’, conjecture and
application.
Physics Engineering Economics
√ √ √
23
24. Energy Sources for Starships
• Chemical: 0.000001 unit, ~13 MJ/kg
• Nuclear Fission: ×1unit, ~82 million MJ/kg
• Nuclear Fusion: ×10 units, ~347 million
MJ/kg
• Nuclear Fission/Fusion
• Antimatter Catalysed Fusion
• Antimatter: ×1,000 unit, 90 billion MJ/kg
• Propellantless Solutions
• Solar Sails
• Laser Sails
• Interstellar Ramjets
• Space Drives & Metric Drives
• Vacuum Energy
• Dark Energy
• Negative Energy
• Warp Drives
24
25. The Physics of Nuclear Fusion
• Sun confines fusion plasma by gravitational field.
• Tokamak uses magnetic field to confine plasma.
• ICF uses inertial mass of material to confine plasma.
• Balance of compression & ignition to deliver fusion energy
to engine.
• Ideal reactions: D(T,He4)n (radioactive) D(He3,He4)p
(charged particle, minimal shielding required).
• D + T He4(3.52MeV) + n(14.06MeV)
• D + D T(1.01MeV) + p(3.03MeV)
• D + D He3(0.82MeV) +n(2.45MeV)
• D + He3 He4(3.67MeV) + p(14.67MeV)
• Li6 + n T + He4 + 4.8MeV
• Li7 + n T + He4 + n - 2.5MeV
25
26. Fusion Triple Product (Lawson Criteria)
nT 10 m sKeV
21 3
For ~10keV plasma
n 10 m s
20 3
Confinement n
Inertial ~1023cm-3 <1ns
Magnetic 10-6cm-3 ~few sec
26
27. National Ignition Facility (US)
• Neodymium glass laser
• Started operation 2009.
• 192 beams
• Deliver 1.8MJ to target.
• Potential output power
20MJ for ns but could
be high as 45MJ.
• Achievable gains >10.
27
28. Project Daedalus (BIS, 1973-1978)
Bond, A et al., “Project Daedalus”, Final
Study Report, JBIS Special Supplement,
1978. Credit: Adrian Mann
28
35. Enzmann Colony Starship (1960s)
Crowl, A, “The Enzmann Starship: History &
Engineering Appraisal”, JBIS, 65, 6, June
2012.
35 Credit: David Hardy
36. World Ships
World Ships (1980s)
Martin, A.R, World Ships – Concept, Cause, Cost, Bond, A & A.R.Martin, World Ships – An Assessment of
Construction and Colonisation, JBIS, 37, pp.243- the Engineering Feasibility, JBIS, 37, pp.254-266, pp.254-
253, pp.243-253, June 1984. 266, June 1984.
36 Credit: Adrian Mann
42. Warp Drive Physics
ds dt [dx vs (t ) f (rs (t ))dt ] dy dz
2 2 2 2 2
Alcubierre, M, The Warp Drive: Hyper-Fast Travel within
General Relativity, Class.Quantum Grav, 11-5, L73-L77, 1994.
42
43. NASA Breakthrough Propulsion Physics Project
1996 - 2002
Three visionary breakthroughs
were identified:
(1) Mass: propulsion that
requires no propellant
(2) Speed: propulsion that
circumvents existing speed
limits
(3) Energy: breakthrough
methods of energy
production to power such
devices.
43
52. I4IS Logo
“Scientia ad sidera”
Knowledge to the Stars
52
53. Mission & Vision
• Mission Statement:
"The mission of the Institute for Interstellar Studies is to
foster and promote education, knowledge and technical
capabilities which lead to designs, technologies or enterprise
that will enable the construction and launch of interstellar
spacecraft."
• Vision Statement:
"We aspire towards an optimistic future for humans on Earth
and in space. Our bold vision is to be an organisation which is
central to catalysing the conditions in society over the next
century to enable robotic and human exploration of the
frontier beyond our Solar System and to other stars, as part
of a long-term enduring strategy and towards a sustainable
space-based economy.
53
54. Web Sites
www.I4IS.org www.interstellarindex.com
54
57. Educational Academy
• Purpose: To build the knowledge and
people capability
• 3 internal students
• 4 ISU Msc students:
• James Harpur, “design of 100 kg interstellar probe”
• Piotr Murzionak, design of an 550-1000 AU interstellar
precursor mission”
• Wei Wang, Review of deceleration options for an interstellar
probe”
• Eric Franks, “Agricultural methods for microgravity
environments”.
57
58. Research & Development
• Purpose: To conduct the fundamental
research, solve the problems, derive
solutions, insights and designs.
• CATSTAR
• OAKTREE
• Bussard
• SENTINEL
• Quantum Light
• Unruh
• BAIR
• Casimir
• GeV
58
59. Enterprise
• Purpose: To develop and spin-out the
technology developments as
innovations, business or enterprise.
• Similar to the Stanford University model of
the 1940s and 1950s when dean of
engineering Frederick Terman encouraged
faculty and graduates to start their own
companies, e.g. Hewlett-Packard, Varian
Associates…Silicon Valley
59
68. CATSTAR PROGRAM
CubeSat Architecture Tests for Space Technology
And Readiness
Goal: To design
5. Mission
concepts and build Appication
4. Orbital
missions cheaply which System
(~$1000,000s)
can demonstrate Demonstrator
(~$100,000s)
interstellar related
technologies using
CubeSat and smaller 3. Engineering
Ground
devices, related Demonstration
architectures. (~$10,000s)
2. Physics
Principles
Validated
(~$1000s)
1. Physics
Principles
Understood
(~$100s)
69. “Travel to the stars will be difficult
and expensive. It will take
decades of time, GW of power, kg
of mass-energy and trillions of
dollars…interstellar travel will
always be difficult and expensive,
but it can no longer be considered
impossible”.
Dr Robert Forward, 1996.
www.i4is.org