Titan an Astrobiological Vision
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En la presente se muestra un poco mas sobre una de las lunas que tiene Saturno, cual es en este caso Titan es importante por sus características atmosféricas pues esta compuesto por Metano, nitrógeno y argón mayoritariamente, también que es de mucho interés para NASA quien esta realizando un seguimiento exhaustivo mediante un sofisticado equipo que órbita Saturno Cassini Huygens
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2) Photos of Earth, the Gulf of Aden, and the International Space Station taken from the ISS.
3) A massive ring system discovered around an exoplanet 200 times larger than Saturn's rings.
4) Cloud formations over the Bering Sea captured by NASA's Aqua satellite.
5) Curiosity rover and Earth at night photographed from the ISS.
Saturn and its Moons
The Cassini spacecraft has captured new images of Saturn and its moons over the past few months. It photographed plumes erupting from Enceladus, a glint of sunlight reflecting off a lake on Titan, and detailed views of the surfaces of moons like Mimas, Tethys, and Dione. Cassini's photos provide striking glimpses of the dynamic Saturn system and its icy, cratered moons over 1 billion kilometers from Earth.
Solar system [Raj Jaiswal]
this power point presentation contain all the description about milky way galaxy & solar system with picture & sound...
by just clicking F11 this PPT will start...
X rays - mission science
- X-rays were discovered in 1895 by Wilhelm Roentgen and have much higher energy and shorter wavelengths than ultraviolet light.
- X-rays can be used to see inside the body by creating detailed images of bones and other dense tissues.
- X-rays are emitted by extremely hot objects like supernovae remnants and accretion disks around black holes, and can provide information about the composition, temperature, and density of celestial environments.
- Telescopes use grazing-incidence mirrors to focus x-rays onto detectors in order to collect and analyze photons from space.
Saturn Gn
Saturn is known for its prominent ring system. Early astronomers like Galileo first observed the rings, though they were not well understood until Christiaan Huygens correctly interpreted them as a ring system in 1659. The Cassini mission has returned stunning images of Saturn and its moons like Titan, greatly increasing scientific understanding of the Saturnian system.
Stage astrofisica 2010- 3. Cassini e il sistema di Saturno - F.Tosi
Stage di astrofisica IASF/IFSI, 3° Edizione
Giorno 1- Lezione 3: La missione Cassini-Huygens, Il Sistema di Saturno
Exploring Solar System
A solar system refers to a star and all the objects that travel in orbit around it. Our solar system consists of the sun - our star - eight planets and their natural satellites (such as our moon); dwarf planets; asteroids and comets. Our solar system is located in an outward spiral of the Milky Way galaxy.
Solar System
The Solar System consists of the Sun and objects that orbit it, including 8 planets, dwarf planets, asteroids, and comets. The inner Solar System contains terrestrial planets like Earth that are composed of rock and metals. The outer Solar System contains gas giants like Jupiter and Saturn that account for most of the mass. Objects follow elliptical orbits around the Sun, with closer objects moving faster according to Kepler's laws of planetary motion. The Solar System is believed to have formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud.
ILOA Galaxy Forum Canada 2015 - Paul Hickson
-- Large optical telescopes on the Moon – Paul Hickson, Professor, Department of Physics and Astronomy, The University of British Columbia.
The Moon offers some unique advantages for future very-large optical telescopes. The airless environment, slow lunar rotation and precession would enable a zenith-pointing telescope, located near one of the lunar poles, to survey a large region of sky and study the epoch of galaxy formation. I will present results from a recent NASA/CSA study that considered the feasibility of lunar liquid-mirror telescopes having apertures in the 20 to 100 metre range.
Astronomy (1)
The document provides information about various astronomical objects including:
- Descriptions of the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune including their distances from the sun, diameters, masses, densities, temperatures, and orbital periods.
- Descriptions of Saturn's rings and Jupiter's moons.
- Information about the sun, moon, stars, asteroids, comets, galaxies, pulsars, and black holes.
Cosmic monster' star spits energy with the force of a billion suns
High energy outbursts in this type of neutron star — a magnetar — are thought to be caused by "starquakes."
Cassini vims hyperspectral_observations_of_the_huygens _landing_site_on_titan
VIMS images of the Huygens landing site on Titan acquired during Cassini flybys in October and December 2004 provide insight into surface features near the landing site with spatial resolutions of 14.4-19 km/pixel. Ratio images of the brightest and darkest spectra in the 2.03 μm window reveal a particularly contrasted structure north of the landing site, consistent with local enrichment in exposed water ice. The images also show a possible 150 km diameter impact crater with a central peak. While scattering from haze particles dominates Titan's spectrum, spectral ratios of bright and dark areas suggest differences in surface composition and/or topography related to DISR images of the site.
Our Solar System
The document provides an overview of our solar system and the universe. It discusses that our solar system formed from a great cloud of gas and dust around 5 billion years ago. It is located within the Milky Way galaxy, which contains over 200 billion stars. Our solar system contains 8 planets orbiting the Sun, along with smaller objects like asteroids, comets, and meteorites. Beyond our solar system, there are other galaxies like the Andromeda galaxy.
Astronomy
The document summarizes key concepts about the sun-earth-moon system from an earth science perspective. It describes how telescopes and space-based tools have enabled the study of electromagnetic radiation and observations of other celestial bodies. It also outlines formation theories for the moon, and explains how the daily motions of the sun, earth and moon influence tides and phases.
Electro magnetic spactrum
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.
University of Arizona Hubble Space Telescope Discoveries
University of Arizona Hubble Space Telescope DiscoveriesUniversity of Arizona Research, Discovery & Innovation
Since NASA launched its Hubble Space Telescope in 1990, space scientists at the University of Arizona in Tucson have used it to expand our knowledge of the Universe time and time again. Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with ...
On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter,
passing less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter’s
poles show a chaotic scene, unlike Saturn’s poles. Microwave sounding reveals weather
features at pressures deeper than 100 bars, dominated by an ammonia-rich, narrow
low-latitude plume resembling a deeper, wider version of Earth’s Hadley cell. Near-infrared
mapping reveals the relative humidity within prominent downwelling regions. Juno’s
measured gravity field differs substantially from the last available estimate and is one
order of magnitude more precise. This has implications for the distribution of heavy
elements in the interior, including the existence and mass of Jupiter’s core. The observed
magnetic field exhibits smaller spatial variations than expected, indicative of a rich
harmonic content.
A Brief History and Research of the Supernova Cas A
A power point presentation I gave at Cal Poly Astronomical Society. The topic is the supernova remnant Cas A.
Ch 1 -the powers of ten
1. The document discusses various units of distance used in astronomy including the astronomical unit (AU), parsec, and light-year.
2. It provides conversions between these units, for example 1 AU = 149,597,870,700 m, 1 parsec = 3.086 x 1016 m, and 1 light-year = 9.460530 x 1015 m.
3. The document also contains information about constellations, galaxies, and how astronomers study distant objects that cannot be touched.
Similar to Titan an Astrobiological Vision (20)
Stage astrofisica 2010- 3. Cassini e il sistema di Saturno - F.Tosi
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Cosmic monster' star spits energy with the force of a billion suns
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Cassini vims hyperspectral_observations_of_the_huygens _landing_site_on_titan
University of Arizona Hubble Space Telescope Discoveries
University of Arizona Hubble Space Telescope Discoveries
Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with ...
Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with ...
A Brief History and Research of the Supernova Cas A
A Brief History and Research of the Supernova Cas A
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Exposición en el seminario Internacional del Colegio de Ingenieros del Perú-Consejo Departamental Arequipa, sobre parte de una investigación en el ecosistema acuático marino del puerto de Ilo, respecto a la contaminación por metales pesados y utilizando la tecnica analitica de espectrofotometria de absorcion atómica y respectiva evaluación con estándares de ECAs-Perú y USEPA.
Proyecto brazo robot mediante algoritmos evolutivos
El presente proyecto es un prototipo que se viene desarrollando en la ciudad de Ilo por parte de un grupo multidisciplinario, como un aporte en la mejora y salud de personas que trabajan segregando residuos sólidos, vemos que este proyecto también se puede aplicar en diferentes escenarios de la industria previo entrenamiento respectivo.
Diseño y Estructura de un Brazo Robot Seleccionador de Objetos
La presentación es la primera etapa sobre diseño y estructura del brazo seleccionador de objetos el cual se enfocara en la selección de residuos sólidos con el fin del cuidado de la salud pública y obtención de materia prima para próximo uso como se explico en el presente evento. producido por EPISI UNAM- ILO.
Ecosistema Acuático del Puerto de Ilo
Se presenta una breve resumen de la investigación científica que se viene desarrollando con información preliminar de los estudios de los ecosistema acuático marinos del puerto de Ilo en conmemoración de un aniversario mas de la Escuela Profesional de Ingeniería Ambiental EPIAM-ILO.
Día Mundial del Agua
Ponencia sobre el día del Agua que fue realizado por el Colegio de Ingenieros del Perú - Arequipa. Proyecto que se realizó y que se viene realizando para conocer la calidad del agua de mar y del ecosistema marino en el puerto de Ilo
Investigación científica en Ingeniería Química
La presentación es una descripción y la importancia de la Ingeniería Química en nuestro planeta y en el dia a dia de nuestra población, en cuanto a las necesidades. el proceso industrial y protección de los recursos y el medio ambiente. Desarrollado en el evento organizado por el Colegio de Ingenieros del Perú - Arequipa, Capitulo de Ingenieria Quimica.
Microplásticos en ecosistemas acuáticos marinos
Presentación que se desarrollo para la población estudiantil y publico en general en la ciudad de Huarmey y por invitación de la SubGerencia de Gestión Ambiental del Municipio Provincial de Huarmey, en favor de concientizar y brindar educación ambiental a la población, gracias por esta oportunidad.
Investigación y tecnología del agua (Continentales y Marino Costeros)
La presente es una breve descripción de lo que se viene realizando en la Universidad Nacional de Moquegua para conocer como estamos en cuanto a la calidad de agua en los diferentes ecosistemas acuáticos y como9 esto sirve como una herramienta para tomar decisiones en las mejoras futras de mano con la sociedad en esta ciudad de Moquegua.
Proyecto de la Calidad de agua en manantiales de chuña
La presente presentación es el trabajo realizado por un grupo de trabajo de Escuela Profesional de Ingeniería Ambiental de la Universidad Nacional de Moquegua, se desarrollo muestreo y monitoreo en el distrito de Ichuña en Sánchez Cerro Moquegua, Perú. Fue realizar análisis de metales pesados en los manantiales de Humalzo, Totorani y Mauri.
El evento del Niño - Enos o Enso
Este documento describe brevemente El Niño Oscilación del Sur (ENSO), un fenómeno climático que ocurre en el Océano Pacífico y afecta el clima globalmente. Explica que se han realizado esfuerzos para determinar la relación entre fases de ENSO y tornados en los Estados Unidos durante los meses de invierno, considerando solo "brotes mayores" de 10 o más tornados. El objetivo no es intentar asociar un ciclo particular de ENSO con eventos de tornado en 45 años.
CLIMATOLOGÍA EN LA FRANJA DESÉRTICA DE ILO-PERU (METEOROLÓGIA Y CLIMA)
El documento presenta información sobre la climatología en la franja desértica de Ilo, Perú. Se registraron datos meteorológicos como temperatura, humedad y punto de rocío en dos puntos de estudio, Las Lomas de Ilo y El Algarrobal, durante dos meses para analizar los parámetros climáticos y su influencia en el clima local. Se utilizaron sensores, un registrador de datos y software para medir y procesar la información meteorológica.
Curva de Abatimiento del CO2
Breve explicación de Cambio Climático; de donde proviene, porque se da y las consecuencias. También desde el punto de vista de la Ingeniería Ambiental como se realiza la aplicación de la encomia ambiental en la valoración en la minimizacion de CO2 o como retribuir por la contaminación atmosférica.
Teoria de Gaia
En esta presentación tenemos el análisis de la Teoría de Gaia establecida por el científico Lovelock el cual nos brinda antecedentes y datos de como el cambio climático se da y viene dando en nuestro planeta Tierra, siendo los compuestos que mas directamente se relacionan con este fenómeno, el aumento del CO2 y los cambios bruscos delos estados del agua el cual es un termo regulador de temperatura en nuestro planeta.
Calentamiento Global
Aquí se hace un análisis sobre el calentamiento global en nuestro planeta o lo que se conoce como aumento de la temperatura en la tierra, según postulado del Dr. Hansen y sus dos puntos de vista las causas. Como parte de la Ingeniería Ambiental nosotros lo analizamos y en parte estamos de acuerdo que la fuente antropológica lo que hace es acelerar los cambios en nuestro clima tal como lo estamos viviendo ahora.
Importancia de las Pampas de la Joya como análogo a Marte
El documento describe la importancia del Desierto de la Joya en Arequipa, Perú como un análogo de Marte. Estudios realizados en el desierto incluyen monitoreo climático de 4 años que muestran temperaturas entre 18.9°C y 35.9°C, radiación solar alta, y humedad relativa baja excepto durante precipitaciones ocasionales. El desierto ofrece un hábitat extremo similar a Marte y se está estudiando para replicar experimentos de posible terraformación en Marte.
Desierto de la Joya Análogo a Marte
La siguiente presentación es un resumen sobre el área de estudio que concierne al desierto de la Joya en Arequipa -Perú.Con imagenes panorámicas y es ecosistema presente en el área,también la climatología y estudios que se realizaron y se continúan haciendo en el desierto de la Joya, Todo esto gracias al grupo multidisciplinario conformado por investigadores nacionales e internacionales.
Contaminacion Ambiental y Mineria
Esta presentación la realice en un forum organizado por el distrito de torata, en el cual se muestra las diferentes formas de contaminación ambiental y como la minería de alguna manera como empresa económicamente activa es buena y como también pueden dañar nuestro medio ambiente si no llevan un control adecuado en sus procesos y mejora del hábitat donde se desarrollan. También se ve que es útil la presencia de un laboratorio de control ambiental para una vigilancia adecuada del medio ambiente.
Horas frío y AG3 en Duraznero
En esta presentación se detalla el trabajo realizado en laboratorio y campo sobre la importancia de horas frió en semillas de frutos para obtener buenos plantones, tambien se logra demostrar como y cuando es bueno o no usar el AG3, el cual es el Ácido Giberelico una hormona que sirve para ayudar al buen desarrollo de los plantones y primordial en monitoreo de temperaturas y humedad relativa para un buen tratamiento de horas frió en semillas de frutas como es el presente estudio.
Plan de Manejo Ambiental - Mitigacion
Este documento presenta un plan de manejo ambiental con enfoque en la mitigación. Describe las medidas de mitigación, compensación, monitoreo e indicadores que se implementarán para reducir los impactos ambientales negativos del proyecto. También incluye secciones sobre gestión de residuos, señalización de obras y el rol del laboratorio ambiental para el monitoreo de variables.
Monitoreo Ambiental - Calidad de Aire
La presente trata sobre Monitoreo Ambiental del Aire, un resumen de la atmósfera de nuestro planeta, parámetros que se miden en el aire y la ley vigente en nuestro país con parámetros que se deben medir para una mejor calidad de vida, también se muestran equipos que se usan para tomar data de diferentes agentes presentes en nuestra atmósfera y en especial el equipo con el que trabajamos para medir material particulado como PM10 Y PM2.5
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Proyecto brazo robot mediante algoritmos evolutivos
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Investigación y tecnología del agua (Continentales y Marino Costeros)
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CLIMATOLOGÍA EN LA FRANJA DESÉRTICA DE ILO-PERU (METEOROLÓGIA Y CLIMA)
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Titan an Astrobiological Vision
- 1. Titan: An astrobiological vision from the Cassini-Huygens data - 2008 RENEE M. CONDORI APAZA ASL – NASA AMES
- 3. Orange and Blue Hazes These views from Cassini look toward the south polar region of Saturn's largest moon, Titan, and show a depression within the moon's orange and blue haze layers near the south pole. The close-up view was captured with the narrow-angle camera. Another view taken a second later with the wide-angle camera is also included here for context. The moon's high altitude haze layer appears blue here whereas the main atmospheric haze is orange. The difference in color could be due to particle size of the haze. The blue haze likely consists of smaller particles than the orange haze. The depressed or attenuated layer appears in the transition area between the orange and blue hazes about a third of the way in from the left edge of the narrow-angle image. The moon's south pole is in the upper right of this image. This view suggests Titan's north polar vortex, or hood, is beginning to flip from north to south.
- 33. DISR instrument DLVS DLIS Imagers Lamp
- 34. Cassini's Superhuman Senses Optical Remote Sensing Mounted on the remote sensing pallet, these instruments study Saturn and its rings and moons in the electromagnetic spectrum. Composite Infrared Spectrometer (CIRS) Imaging Science Subsystem (ISS) Ultraviolet Imaging Spectrograph (UVIS) Visible and Infrared Mapping Spectrometer (VIMS) Fields, Particles and Waves These instruments study the dust, plasma and magnetic fields around Saturn. While most don't produce actual "pictures," the information they collect is critical to scientists' understanding of this rich environment. Cassini Plasma Spectrometer (CAPS) Cosmic Dust Analyzer (CDA) Ion and Neutral Mass Spectrometer (INMS) Magnetometer (MAG) Magnetospheric Imaging Instrument (MIMI) Radio and Plasma Wave Science (RPWS) Microwave Remote Sensing Using radio waves, these instruments map atmospheres, determine the mass of moons, collect data on ring particle size, and unveil the surface of Titan. Radar Radio Science (RSS)