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The Universe - UNC Charlotte Pages
The Universe - UNC Charlotte Pages

... up its surface area (space) increases with time. The clusters of galaxies do not increase in size. They get further apart but do not move through space. ...
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... planets orbit the sun and moons orbit planets. It is gravity that keeps an object in orbit!” 2. “The Earth is the center of the universe, and all of the planets and stars orbit our planet. How do I know? Well, my theory predicts the motion of the planets better than any other theory of my day.” ...
Astronomy Midterm Review Sheet
Astronomy Midterm Review Sheet

... c. An object in motion remains in motion. d. The parabola is a kind of conic section. 58. What object is located at one focus of the orbit of the planet Mars? a) the Sun b) the Earth c) Mars d) Jupiter 59. According to Kepler’s laws, a planet moves fastest in its orbit when it is a) nearest the Eart ...
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... easier to make, requiring only three spherical surfaces to be ground and polished. The secondary mirrors of Maksutovs are usually smaller than those on Schmidt-Cassegrains Steve Edberg has a variety of telescopes so he can choose the right one for every occasion. His wife is not amused. ...
Sirius Astronomer - Orange County Astronomers
Sirius Astronomer - Orange County Astronomers

... jets. A Chandra observation made 2 months before the ultrafast wind was seen showed no evidence of the wind, so the wind apparently turns on and off over time. Astronomers believe that magnetic fields in the disks of black holes are responsible for producing both the winds and jets. Changing conditi ...
Fundamental properties of the Sun - University of Iowa Astronomy
Fundamental properties of the Sun - University of Iowa Astronomy

... • A wind past the Earth at 400 km/sec • The Sun is “melting away” • Density 19 orders of magnitude less than atmosphere • A medium for solar events • May have “sandblasted” the early atmosphere of Mars ...
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... 56. The planets formed into two main groups: the inner terrestrial planets and the outer Jovian planets. Which of the following is NOT characteristic of the formation sequence of the terrestrial planets? a. Heavy elements condense to form grains and then planetesimals. b. Planetesimals coalesce and ...
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... one must take the telescopes outside of the atmosphere. Such instruments have been developed to study infrared, ultraviolet, X-ray and gamma rays. Infrared and ultraviolet telescopes look fairly similar to optical telescopes, but there are some important differences. A special problem for infrared t ...
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NIE10x301Sponsor Thank You (Page 1)

... Jupiter, and the phases of Venus and craters on the moon. These observations began the human exploration of the Universe with the aid of telescopes and the modern science of Astronomy. With even the smallest telescope, or possibly an ordinary pair of binoculars, you may be able to see the four large ...
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English version

... principal center of activity in observational solar physics, for over a century. At present, the main facility is the solar tower tunnel telescope fitted with a spectrograph, which is in regular use since 1962; a spectro-polarimeter has also been added. This observatory has a unique collection of th ...
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Science Overview

... Kepler and HARPS • Kepler yields 20 times better photometry • HARPS yields 20 times better RV • Kepler launch now 16 February 2009 – First candidates 9 months later – HARPS ready for 2010 observing season ...
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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.
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