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The Ever Expanding Universe
The Ever Expanding Universe

... The distances to stars and galaxies are approximate measures that are often revised especially if they are far away. Our understanding of the Universe depends upon accurate mapping of every structure in the Universe and was begun by the Greeks, Persians and Indians thousand of years ago! Measuring t ...
Eyles, Bunker, Ellis et al. astro-ph/0607306 Eyles, Bunker, Ellis et al
Eyles, Bunker, Ellis et al. astro-ph/0607306 Eyles, Bunker, Ellis et al

... -Have shown that some z=6 I-drops have old stars & large masses (subsequently confirmed by H. Yan et al) -Hints that there may be z>6 galaxies similar (Egami lens). Mobasher source - z=6.5??? (may be lower-z) -Turn now to larger samples, to provide stellar mass density in first Gyr with Spitzer -- ...
Name ______KEY Date Core ______ Study Guide Galaxies and the
Name ______KEY Date Core ______ Study Guide Galaxies and the

... When did the Big Bang happen and what has happened since? The big bang theory is theorized to have happened 14 billion years ago when the universe suddenly began to expand from one merged mass of matter or substance. At that time, all matter was dense and hot and the universe developed in less than ...
how do the planets affeCt earth?
how do the planets affeCt earth?

... The end of the solar system In about 5 billion years, the Sun will grow into a red giant star. It will become about eight times larger than it is today. When this happens, the inner planets will be destroyed by its heat. The outer planets will move further out into space. The red giant will slowly b ...
- BIO Web of Conferences
- BIO Web of Conferences

etlife_exoplanets - University of Glasgow
etlife_exoplanets - University of Glasgow

... We can tell that planets are there by the effect they have on their star. ...
Folie 1 - univie.ac.at
Folie 1 - univie.ac.at

... typical time scales for their variability ranging from an hour to several weeks and aiming for a frequency resolution sufficient for asteroseismology, BRITE-Constellation expects to observe on average 20 stars simultaneously. ...
Lecture 2 - University of Chicago, Astronomy
Lecture 2 - University of Chicago, Astronomy

... in the telescope, but stars did not; observed all four phases of the Venus (gibbous phases could not be explained by the Ptolemaic model); discovered four largest satellites of Jupiter; they are still called Galilean moons; this was another blow to the dying Ptolemaic system. Galileo resolved the Mi ...
Keywords:​ Pluto, New Horizon Hubblecast Episode
Keywords:​ Pluto, New Horizon Hubblecast Episode

... kilometres, and the planet’s polar regions as well as some  large bright spots are visible.  ...
Uranus Questions
Uranus Questions

... some of the other planets; they just didn't know that they were planets. By the time of the ancient Greeks, some logically-minded people had figured out that not everything up there was a star. Stars stayed in one place, but other heavenly bodies, such as planets, moved. In this way, they discovered ...
Welcome to the Magic Valley Astronomical Society Pomerelle
Welcome to the Magic Valley Astronomical Society Pomerelle

... mission to look deep beneath the planet's swirling curtain of clouds to find out what lies beneath. The answer might confirm theories about how the solar system formed, or it may change everything we thought we knew. "The special thing about Juno is we're really looking at one of the first steps, th ...
ppt
ppt

... -Have shown that some z=6 I-drops have old stars & large masses (see also talk by H. Yan) -Hints that there may be z>6 galaxies similar (Egami lens). Mobasher source - z=6.5??? (may be lower-z) -Turn now to larger samples, to provide stellar mass density in first Gyr with Spitzer -- In Stark, Bunk ...
Portable Speckle Interferometry Camera Checkout at Kitt Peak
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... nights on the 2.1m telescope at Kitt Peak National Observatory for double star speckle interferometry using a portable camera. As described in the proposal, binary orbits, when combined with parallaxes, yield dynamical masses, while photometry of the components restrains astrophysical models. Both a ...
Unit E: Section 2.0
Unit E: Section 2.0

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... 17. Explain the big bang theory in as much detail as possible. Make sure you answer the following questions: 1. Is the universe expanding or getting smaller? 2. What evidence did the WMAP provide scientists about the big bang? 3. Is the universe cooling or getting hotter? Less or more dense? 4. How ...
Jun 2015 - Astronomical Society of Northern New England
Jun 2015 - Astronomical Society of Northern New England

... atmosphere's airflow all in one swoop. It's also the best way, so long as you're up at high enough altitudes, to view an entire 50 percent of Earth all at once. And if you place your observatory at just the right location, you can observe the same hemisphere of Earth continuously, tracking the chang ...
August - Magic Valley Astronomical Society
August - Magic Valley Astronomical Society

... radiant is low in the north-northeast, so the meteors strike the upper atmosphere at a low angle, therefore we see comparatively few of them. As the night advances, the radiant rise higher in the northeast, the meteors arrive more nearly straight down, so we see more of them. The Perseid meteor show ...
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Comet ISON keeps observers guessing

... how they behave, especially compared to predictions of their behaviour; comet Kohoutek (C/1969 O1) in 1969 is in the mind of many comet observers, since it was widely talked up as a comet of the century but proved to be less than spectacular. Comet ISON has been suggested as a naked-eye object for l ...
BRC_prop1 - CoolWiki
BRC_prop1 - CoolWiki

... spectrum. They will compare images obtained by IRAC, MIPS and IRAS to learn about spatial resolution. Evidence will be presented to help students understand how the universe is changing, how stars and planets are forming, and how stars evolve from birth to eventual death. Combining images at differe ...
Space exploration - Menihek Home Page
Space exploration - Menihek Home Page

... monkeys, chimpanzees, dogs and cats (mammals were preferred because they most resembled people). Rockets travel by thrust (think of letting go of a balloon that you’ve almost completely blown up). As the fuel on a rocket gets used up, parts of the rocket’s propulsion system break off from the rocket ...
S E N S ` 2 0 0 6
S E N S ` 2 0 0 6

... last year they find at least 192 planets around different kind of stars and star systems [1, 2, 3, 4]. Most of them are not alone but in planetary systems like our Solar system (not less then 155 planetary systems). Protoplanetary disks have been observed around several young stars in our galaxy, th ...
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... exciting astronomical discoveries of recent times: Proxima b, the potentially habitable planet closest to Earth; and TRAPPIST-1, a system of seven Earth-size planets not far from our own Solar System which may have the right conditions for life. De Zeeuw, who in September this year will be succeeded ...
Astronomy Assignment #1
Astronomy Assignment #1

... To account for giant planets in very close non-circular high-eccentricity orbits one might hypothesize that two Jovain planets in the outer part of the nebula had a close encounter – not a collision, but a near miss. Simulations indicate that two jovian planets approaching within 1 AU of each other ...
May 2014
May 2014

... – and blue/red shift of the star's light), and transiting planets. The Kepler telescope used the dip-in-light transit method for finding planets. This method is very limited, as the planets' orbit have to be in line with our line of sight. (If the moon was perfectly in line with Earth's orbit with t ...
Hubble - STScI
Hubble - STScI

... myriad of stars in our Milky Way Galaxy, he launched a revolution that changed our view of an Earth-centered universe. The launch of NASA’s Hubble Space Telescope aboard the space shuttle Discovery 15 years ago initiated another revolution in astronomy. For the first time, a large telescope that see ...
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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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