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ASTR100 Fall 2009: Exam #2 Review Sheet EXAM IS THURSDAY
ASTR100 Fall 2009: Exam #2 Review Sheet EXAM IS THURSDAY

... 3] What color of visible light has the most energy? ________ Why? ________________ 4] Name the four ways light interacts with matter: _______, _______, _______, ______. 5] What type of spectrum will a neon light produce? ____________________________ 6] What type of spectrum will a regular filament l ...
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Astronomy Tools

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Microscopy - Steilacoom High School
Microscopy - Steilacoom High School

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February 2008

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The Supernova`s Secrets Cracked at Last? Most stars end their lives
The Supernova`s Secrets Cracked at Last? Most stars end their lives

... The Supernova's Secrets Cracked at Last? Most stars end their lives in a whimper — our own sun will almost certainly be one of them — but the most massive stars go out with an impressive bang. When that happens, creating what's known as a Type II supernova, the associated blast of energy is so brill ...
supplemental educational materials PDF
supplemental educational materials PDF

... Jupiter’s red spot is the most noticeable feature on the planet. It is a giant, spinning storm that has been raging for at least a hundred years — perhaps since telescopes were first used to study celestial objects. Scientists have marveled at the storm’s ability to survive, but they believe the spo ...
Temporal and Special Variance of chemical species in the
Temporal and Special Variance of chemical species in the

... Description of the potential science / science goals: Observation of integrated light across moon and Mercury with observation of Mercury magnetotail. Determination of exosphere composition to include, especially, atomic lines (sodium, potassium, calcium, hydrogen…). Daytime observations from Antarc ...
Study Guide for Exam 1 Astro 4 Spr`17
Study Guide for Exam 1 Astro 4 Spr`17

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Big Bang

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Astronomy - SAVE MY EXAMS!

... (a) Complete the sentence by putting a cross ( ) in the box next to your answer. The telescope named after Herschel detects infrared radiation. Herschel is a suitable name for this infrared telescope because ...
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Sirius Astronomer - Orange County Astronomers

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Chapter 11

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Another Earth in the Universe
Another Earth in the Universe

... large stars and therefore are the best candidates for planetary systems in which life could be present. In fact, for biological evolution and for biochemical reactions to take place, very long periods of time are required, longer than the average age of the large stars. Furthermore, M dwarfs are ver ...
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Space Part2

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James Webb Space Telescope
James Webb Space Telescope

... The Mirrors Ball Aerospace has teamed with NGST on a telescope design with a primary mirror that is 6.5 meters in diameter. The large, light-collecting area of this mirror allows superior viewing of extremely faint targets. Additional mirrors within the telescope remove residual wave-front errors an ...
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to the Stars and Constellations Fact

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Make your own Telescope

... 1. Add the lengths of the two lenses. Your cardboard tubes will need to be able to extend to at least this length. 2. Make a cardboard tube 10cm in length from the black cardboard. Use blu-tac to secure the largest convex lens in the end of the tube. 3. To calculate the length for the second cardboa ...
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Temperature, df/f

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dobson space telescope the future of microsat based

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Frank Drake

... Before we can talk about life on other worlds, we probably need to define what we mean by life. I don’t think you can assume that life anywhere in the galaxy is just like life on Earth that it has the same kind of DNA. Some scientists have come up with a list of the characteristics of life: 1. Life ...
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Jodrell Bank Discovery Centre Scouts

... Find the dome with two planets orbiting a star Exoplanets are planets outside our solar system, orbiting around other stars. 12. The amount of light from the star is being measured by a camera (in the red circle) and being shown on screen. What happens to the light level when a planet passes between ...
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prime focus

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Rocky Planets Gas Giants

... Comets sometimes burst into pieces when the Sun's heat turns their ice into water vapor. By studying these chunks, astronomers can compare the material at the center of a comet with material at its surface. The scientists expected that a comet's center would look different from its surface. That's b ...
Light and Telescopes - Otterbein University
Light and Telescopes - Otterbein University

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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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