• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
How the Hubble Telescope Will Look at the Moon to See Venus
How the Hubble Telescope Will Look at the Moon to See Venus

... May 07 - Comet 123P/West-Hartley Closest Approach To Earth (2.094 AU) May 07 - Asteroid 3 Juno Occults UCAC2 30551972 (11.8 Magnitude Star) May 07 - Asteroid 2012 HL Near-Earth Flyby (0.054 AU) May 07 - Asteroid 12524 Conscience Closest Approach To Earth (1.431 AU) May 07 - Asteroid 1134 Kepler Clos ...
Astronomy Journals, Physics 1040
Astronomy Journals, Physics 1040

... brighter than any part of the galaxy and as it brightens it may outshine billions of stars in M82. The star explosion happened on January 22, also because this new supernova is twelve million light years away this star actually exploded twelve million years ago. But we are only getting a glimpse of ...
pptx
pptx

... organism on a planet. If so, then fi=1. But for 2.5 billion years, life on Earth did not evolve past single-celled organisms. Perhaps the development of complex (and intelligent) life is very rare. In that case, fi<<1. ...
ROBAST: Development of a Non-Sequential Ray
ROBAST: Development of a Non-Sequential Ray

... hexagonal light concentrator for Cherenkov telescopes. In addition to conventional Winston cone designs, light concentrators with Bézier curve surfaces (hereafter Okumura cones [10]) can be modeled and simulated by ROBAST. Figure 2(a) illustrates a ROBAST model of an Okumura cone and simulated photo ...
Habitable worlds with JWST: transit spectroscopy of the TRAPPIST
Habitable worlds with JWST: transit spectroscopy of the TRAPPIST

... telescope at La Silla observatory. It was designed for detection and characterisation of exoplanets, as well as observations of small solar system bodies. The recent discovery of the TRAPPIST-1 planetary system (Gillon et al. 2016) has provided not one, but three, potential targets for JWST follow u ...
Lesson 0: What is progress
Lesson 0: What is progress

... Brahe was one of the best observational astronomers that ever lived. He made the most precise observations that had yet been made by devising the best instruments available before the invention of the telescope, and His observations of planetary motion, particularly that of Mars, provided the crucia ...
The 1.5 meter solar telescope GREGOR
The 1.5 meter solar telescope GREGOR

... granulation – at the surface. Kilogauss magnetic flux concentrations are observed in granular lanes. According to numerical simulations, their spatial scales are of the order of 100 km, or below (Grossmann-Doerth et al. 1998; Hasan et al. 2005). Lagg et al. (2010) investigated the properties of magn ...
Test - Scioly.org
Test - Scioly.org

... c. Reflected starlight at optical bands and the planet’s radiation in infrared wavelengths  d. Reflected starlight in infrared wavelengths and the planet’s radiation in optical bands  15. Imagine that one of your astronomy “apprentices” is calculating the temperature of a  planet that forms from the ...
Slides
Slides

Exploring Space—The Universe: The Vast
Exploring Space—The Universe: The Vast

... star to our planet besides the sun? (Proxima Centauri.) How far away is Proxima Centauri from our planet? (Proxima Centauri is 4.3 light-years, or 26 trillion miles, away from Earth.) 3. Discuss with students the location of the solar system within the Milky Way galaxy. What are the three types of g ...
Coordinate Systems for Astronomy or: How to get
Coordinate Systems for Astronomy or: How to get

... The world is divided into Time Zones; 15 degrees change in longitude is equivalent to an hour's change in time. South Africa is roughly 30 degrees east of Greenwich, and so South African Standard Time (SAST) is set to be 2 hours ahead of UTC. Our “year” is technically the Earth's “tropical period”. ...
Northrop Grumman Space Primer
Northrop Grumman Space Primer

... Looking up at the moon, we really see it as it was one second ago, because it takes light about one second to travel from the lunar surface to Earth. Although light travels at the incredible speed of about 187,000 miles per second, it takes just over eight minutes for light to reach us from the more ...
newsletter - Thanet Astronomy Group
newsletter - Thanet Astronomy Group

... direction visible from the side of the Earth that faces away from the Sun, the planets can be observed in the night sky all at the same time. This is exactly what is happening now. The planets that have aligned are Mercury, Venus, Mars, Jupiter and Saturn. These are the five planets that are visible ...
GREGOR Upgrade of the GCT on Teneriffe with a 1.5m Solar
GREGOR Upgrade of the GCT on Teneriffe with a 1.5m Solar

... – evacuated coudé path* – lightweight optics – lightweight structure ...
Two Looks at the Visual and Imaging Perfomance of the VISAC
Two Looks at the Visual and Imaging Perfomance of the VISAC

... for another time. The VC200L is an excellent visual scope as well as imaging platform. Once cooled and set up properly, the scope delivers sharp, low power images, bright objects with crisp stars, and very good high power images of double stars, carbon stars, and most every other deep sky object I p ...
Between the Stars: Gas and Dust in Space
Between the Stars: Gas and Dust in Space

... To understand how stars form, we need to know the raw material from which they are made All the gas and dust material that lies in the region between stars is referred to as interstellar matter The entire collection of interstellar matter is called the interstellar medium The interstellar medium acc ...
to access chapter 16
to access chapter 16

... are launched into space where conditions are always clear and dark, perfect for stargazing around the clock! Space telescopes include the Hubble and the Chandra X-ray Observatory. The Arecibo radio telescope in Puerto Rico is the largest single-dish radio telescope in the world. It receives radio wa ...
A-level Physics A Question paper Unit 05 - Section 2A
A-level Physics A Question paper Unit 05 - Section 2A

... l You must answer the questions in the spaces provided. Do not write outside the box around each page or on blank pages. l Do all rough work in this book. Cross through any work you do not want to be marked. ...
electronic imaging in
electronic imaging in

... silicon, there is germanium, gallium arsenide, indium antimonide, and several other materials with these properties. Semiconductors can be used to manufacture a host of low-power micro-electronic components including amplifiers, all sorts of logic units, computer memory, very complex chips called mi ...
PDF format
PDF format

... a)  We see young star clusters with gas and dust around them. b)  Infrared and microwave telescopes let us see protostars inside dust clouds. c)  Computer models predict that if a cloud has enough mass, it will contract, heat up, and form a star. d)  The Hubble Telescope lets us watch stars form bef ...
The future of gamma-ray astronomy
The future of gamma-ray astronomy

... 2743 m altitude) using two bare faced PMTs (EMI 9545B) separated by 1 m and pointing up-wards in the sky (which may be likened to a wide angle telescope with a viewing angle of w.r.t. zenith) in the drift scan mode. In this mode the telescope is kept stationary, and the sky is scanned as Earth rotat ...
XMM - advanced X-ray Astronomy school - X
XMM - advanced X-ray Astronomy school - X

... The size of the PSF increases with increasing off-axis angle. This effect is energy ...
Galaxy1
Galaxy1

... • And remember, the Sun and solar system is moving 220 km/s. That is 528,000 miles/hour! • At that speed it would take 2 minute, 43 seconds to fly around the Earth. • Our Milky Way galaxy and the Andromeda galaxy are going to collide in the future. It will take about 7 to 8 billion years to reach An ...
No Slide Title
No Slide Title

... Several new detections from long exposure ...
Temperate Earth-sized planets transiting a nearby ultracool
Temperate Earth-sized planets transiting a nearby ultracool

... Griep for assistance with the SpeX observations; UKIRT staff scientists W. Varricatt & T. Kerr, telescope operators S. Benigni, E. Moore and T. Carroll, and Cambridge Astronomy Survey Unit (CASU) scientists G. Madsen and M. Irwin for assistance with UKIRT observations; the European Southern Observat ...
< 1 ... 80 81 82 83 84 85 86 87 88 ... 214 >

Spitzer Space Telescope



The Spitzer Space Telescope (SST), formerly the Space Infrared Telescope Facility (SIRTF), is an infrared space observatory launched in 2003. It is the fourth and final of the NASA Great Observatories program.The planned mission period was to be 2.5 years with a pre-launch expectation that the mission could extend to five or slightly more years until the onboard liquid helium supply was exhausted. This occurred on 15 May 2009. Without liquid helium to cool the telescope to the very low temperatures needed to operate, most of the instruments are no longer usable. However, the two shortest-wavelength modules of the IRAC camera are still operable with the same sensitivity as before the cryogen was exhausted, and will continue to be used in the Spitzer Warm Mission. All Spitzer data, from both the primary and warm phases, are archived at the Infrared Science Archive (IRSA).In keeping with NASA tradition, the telescope was renamed after its successful demonstration of operation, on 18 December 2003. Unlike most telescopes that are named after famous deceased astronomers by a board of scientists, the new name for SIRTF was obtained from a contest open to the general public.The contest led to the telescope being named in honor of astronomer Lyman Spitzer, who had promoted the concept of space telescopes in the 1940s. Spitzer wrote a 1946 report for RAND Corporation describing the advantages of an extraterrestrial observatory and how it could be realized with available or upcoming technology. He has been cited for his pioneering contributions to rocketry and astronomy, as well as ""his vision and leadership in articulating the advantages and benefits to be realized from the Space Telescope Program.""The US$800 million Spitzer was launched from Cape Canaveral Air Force Station, on a Delta II 7920H ELV rocket, Monday, 25 August 2003 at 13:35:39 UTC-5 (EDT).It follows a heliocentric instead of geocentric orbit, trailing and drifting away from Earth's orbit at approximately 0.1 astronomical unit per year (a so-called ""earth-trailing"" orbit). The primary mirror is 85 centimeters (33 in) in diameter, f/12, made of beryllium and is cooled to 5.5 K (−449.77 °F). The satellite contains three instruments that allow it to perform astronomical imaging and photometry from 3 to 180 micrometers, spectroscopy from 5 to 40 micrometers, and spectrophotometry from 5 to 100 micrometers.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report