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MSL final assembly 2011-7372.jpg

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MSL final assembly 2011-7372.jpg

CAPE CANAVERAL, Fla. – In the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida, all elements of NASA's Mars Science Laboratory (MSL) mission have come together. The top portion is the cruise stage, next, the aeroshell, (containing the compact car-sized rover Curiosity), and on the bottom, the heat shield. The rover Curiosity has 10 science instruments designed to search for evidence on whether Mars has had environments favorable to microbial life, including chemical ingredients for life. The unique rover will use a laser to look inside rocks and release its gasses so that the rover’s spectrometer can analyze and send the data back to Earth. Launch of MSL aboard a United Launch Alliance Atlas V rocket is scheduled for Nov. 25 from Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida. For more information, visit http://www.nasa.gov/msl .

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Mars Science Laboratory (MSL) spacecraft launches.jpg

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Mars Science Laboratory (MSL) spacecraft launches.jpg

CAPE CANAVERAL, Fla. -- With NASA's Mars Science Laboratory (MSL) spacecraft sealed inside its payload fairing, the United Launch Alliance Atlas V rocket rides smoke and flames as it rises from the launch pad at Space Launch Complex-41 on Cape Canaveral Air Force Station in Florida at 10:02 a.m. EST Nov. 26. MSL's components include a car-sized rover, Curiosity, which has 10 science instruments designed to search for signs of life, including methane, and help determine if the gas is from a biological or geological source.

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MSL Capsule.jpg

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MSL Capsule.jpg

This image from July 2008 shows the aeroshell for NASA's Mars Science Laboratory while it was being worked on by spacecraft technicians at Lockheed Martin Space Systems Company near Denver. This hardware was delivered in early fall of 2008 to NASA's Jet Propulsion Laboratory, Pasadena, Calif., where the Mars Science Laboratory spacecraft is being assembled and tested. The aeroshell encapsulates the mission's rover and descent stage during the journey from Earth to Mars and shields them from the intense heat of friction with that upper atmosphere during the initial portion of descent. The aeroshell has two main parts: the backshell, which is on top in this image and during the descent, and the heat shield, on the bottom. The heat shield in this image is an engineering unit for testing. The heat shield to be used in flight will be substituted later. The heat shield has a diameter of about 15 feet. For comparison, the heat shields for NASA's Mars Exploraton Rovers Spirit and Opportunity were 8.5 feet and the heat shields for the Apollo capsules that protected astronauts returning to Earth from the moon were just under 13 feet. In addition to protecting the Mars Science Laboratory rover, the backshell provides structural support for the descent stage's parachute and sky crane, a system that will lower the rover to a soft landing on the surface of Mars. The backshell for the Mars Science Laboratory is made of an aluminum honeycomb structure sandwiched between graphite-epoxy face sheets. It is covered with a thermal protection system composed of a cork/silicone super light ablator material that originated with the Viking landers of the 1970s. This ablator material has been used on the heat shields of all NASA Mars landers in the past, but this mission is the first Mars mission using it on the backshell. The heat shield for Mars Science Laboratory's flight will use tiles made of phenolic impregnated carbon ablator. The engineering unit in this image does not have the tiles.

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MSL landing.jpg

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MSL landing.jpg

Entry, descent, and landing for the Mars Science Laboratory mission will break down into four parts: Guided Entry, Parachute Descent, Powered Descent and Sky Crane.

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Voyager Captures Sounds of Interstellar Space.webm

Космос · Video

Voyager Captures Sounds of Interstellar Space.webm

NASA's Voyager 1 spacecraft captured these sounds of interstellar space. Voyager 1's plasma wave instrument detected the vibrations of dense interstellar plasma, or ionized gas, from October to November 2012 and April to May 2013. The graphic shows the frequency of the waves, which indicate the density of the plasma. Colors indicate the intensity of the waves, or how "loud" they are. Red indicates the loudest waves and blue indicates the weakest. The soundtrack reproduces the amplitude and frequency of the plasma waves as "heard" by Voyager 1. The waves detected by the instrument antennas can be simply amplified and played through a speaker. These frequencies are within the range heard by human ears. Scientists noticed that each occurrence involved a rising tone. The dashed line indicates that the rising tones follow the same slope. This means a continuously increasing density. When scientists extrapolated this line even further back in time (not shown), they deduced that Voyager 1 first encountered interstellar plasma in August 2012. The Voyager spacecraft were built and continue to be operated by NASA's Jet Propulsion Laboratory, in Pasadena, Calif. Caltech manages JPL for NASA. The Voyager missions are a part of NASA's Heliophysics System Observatory, sponsored by the Heliophysics Division of the Science Mission Directorate at NASA Headquarters in Washington. For more information about Voyager, visit: http://www.nasa.gov/voyager and http://voyager.jpl.nasa.gov . Credit: NASA/JPL-Caltech/University of Iowa

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Journey to the Center of the Galaxy.webm

Космос · Video

Journey to the Center of the Galaxy.webm

Video Credit: ESO/MPE/Nick Risinger (skysurvey.org)/VISTA/J. Emerson/Digitized Sky Survey 2 Details: http://www.eso.org/public/videos/eso1151d/ Details: https://apod.nasa.gov/apod/ap181229.html

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Fly Over Dwarf Planet Ceres.webm

Космос · Video

Fly Over Dwarf Planet Ceres.webm

A new video animation of dwarf planet Ceres, based on images taken by NASA's Dawn spacecraft, provides dramatic flyover views of this heavily cratered, mysterious world. The images come from Dawn's first mapping orbit at Ceres, at an altitude of 8,400 mile (13,600 kilometers), as well as navigational images taken from 3,200 miles (5,100 kilometers) away. The images provided information for a three-dimensional terrain model. The vertical dimension has been exaggerated by a factor of two, and a star field has been added in the background. http://www.jpl.nasa.gov/video/details.php?id=1380 http://apod.nasa.gov/apod/ap150610.html

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MESSENGER False Color Mercury Globe Spin.webm

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MESSENGER False Color Mercury Globe Spin.webm

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?page=1&gallery_id=2&image_id=1085&keyword=73&search_cat=

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Mars at Closest Approach 2016.webm

Космос · Video

Mars at Closest Approach 2016.webm

Mars at Closest Approach 2016 Copyright: Jesús Santos Garzás Details: Astronomy Picture of the Day (APOD): 2016 August 9 Details: http://apod.nasa.gov/apod/ap160809.html

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A Powerful Solar Flare.webm

Космос · Video

A Powerful Solar Flare.webm

Credit: SOHO Consortium, LASCO, ESA, NASA Details: https://sohowww.nascom.nasa.gov/hotshots/2003_10_28/ Details: https://apod.nasa.gov/apod/ap031029.html Comments: http://asterisk.apod.com/discuss_apod.php?date=180902

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Atmospheric erosion at Venus in the HYB simulation.webm

Космос · Video

Atmospheric erosion at Venus in the HYB simulation.webm

Escaping planetary atomic oxygen ions (O+) viewed by a virtual spacecraft orbiting around Venus in the HYB simulation. The colouring on two perpendicular planes and on a spherical shell just above the planet give the density of oxygen ions in a logarithmic scale (red: high density; dark blue: low density). The density of white dots gives the density of the oxygen ions in 3-dimensional space. Note how the escaping oxygen ions form an ion tail behind the planet. (Animation by R. Jarvinen/FMI).

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Magnetic D component at the Earth's surface (AE Map) 1590-1990.webm

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Magnetic D component at the Earth's surface (AE Map) 1590-1990.webm

https://en.wikipedia.org/wiki/Geomagnetic_secular_variation Four centuries of geomagnetic secular variation from historical records Jackson, A., Jonkers, A. R. T. and Walker, M. R. Phil. Trans. Roy. Soc. A (2000) Vol. 358, pp957-990 Some of the data and modelling procedures were also described in the earlier papers: Time-dependent mapping of the magnetic field at the core-mantle boundary Bloxham, J. and Jackson, A. Journal of Geophysical Research Vol. 97, B13, pp.19537-19563 Geomagnetic Secular Variation Bloxham, J., Gubbins, D. and Jackson, A. Phil. Trans. Roy. Soc. A (1989) Vol. 329 pp415-502

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Mars Fleet and Comet Siding Spring.webm

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Mars Fleet and Comet Siding Spring.webm

Flying past comet Siding-Spring the Mars orbiting fleet is faded on while Siding Spring passes very close to Mars.

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Enrique Chaudet.jpg

Космос · Photo

Enrique Chaudet.jpg

Enrique Chaudet (8/12/1881 Francia - 29/6/1967 Córdoba, Argentina) empleado del Observatorio Nacional Argentino (hoy OAC) entre 1911 y 1930. Previo a su ingreso al observatorio de Córdoba, trabajó durante unos meses en el Observatorio de La Plata efectuando cálculos. Entre el 18 de febrero y 10 de agosto de 1911, a modo de colaboración, realiza tareas en la estación de Oncativo del observatorio platense. En 1912 actúa como computador y posteriormente es designado astrónomo de tercera. Realizando numerosos trabajos relacionados con observaciones de cometas y eclipses solares. Tiene a su cargo la expedición a Venezuela para observar el eclipse de 1916. Realiza observaciones con el círculo meridiano y para la Córdoba Durchmusterung. Renuncia a su puesto el 12 de diciembre de 1930, como consecuencia de las desinteligencias que tiene con el director Charles Perrine. Pasa a trabajar en la Oficina Meteorológica.

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Nélida Keller.jpg

Космос · Photo

Nélida Keller.jpg

Nélida Keller (2/8/1909 Córdoba - ¿?) Calculista Ayudante del Observatorio Nacional Argentino - Observatorio Astronómico de Córdoba. Empleada entre 1929 y 1974.

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David Mac Leish.jpg

Космос · Photo

David Mac Leish.jpg

David Mac Leish (8/6/1907 Córdoba - 17/4/1971 Córdoba) ayudante fotógrafo del Observatorio Astronómico de Córdoba, realizó cientos de fotografías con el telescopio de 1,5 metros de la Estación Astrofísica de Bosque Alegre. Fue un valioso y preciado miembro de la institución. https://historiadelaastronomia.wordpress.com/2014/05/04/david-mc-leish/

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