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Phys133 SAMPLE questions for MidTerm#1
Phys133 SAMPLE questions for MidTerm#1

... B) It is the star straight overhead. C) It appears very near the north celestial pole. D) It can be used to determine your longitude on Earth. E) It is the star directly on your northern horizon. ...
PPT Format - HubbleSOURCE
PPT Format - HubbleSOURCE

... a system of two objects in space (usually stars), which are so close that their gravitational interaction causes them to orbit around their common center of mass. ...
Skymapper and Kepler K2: Finding the Origin of Hot Gas Giants
Skymapper and Kepler K2: Finding the Origin of Hot Gas Giants

... determine which stars are young. • Data/pretty images prior to May 1 would really help the proposal for K2 targets! • This is standard “fast” survey data. ...
Watch the episode titled “The Milky Way” from the series “The
Watch the episode titled “The Milky Way” from the series “The

... What do astronomers think came first, the galaxy or the black hole? Besides being sucked into the black hole, what else is happening at the edges of a black hole? Once formed at the edge of a black hole, what is likely to happen to that star? About how many times has our solar system been orbited ar ...
Slide 1
Slide 1

... Basic Facts ...
CT9
CT9

... Astronaut Dave Bowman is standing in the centrifuge of the spaceship Discovery. He drops his pen and observes it fall to the floor. Which statement below is most accurate? A: After Bowman releases the pen, the net force on the pen is zero. B: The pen falls because the centrifugal force pulls it towa ...
December 2015 - Hermanus Astronomy
December 2015 - Hermanus Astronomy

... the ‘Bagnold Dunes’, which skirt the north-western flank of Mount Sharp. No Mars rover has previously visited a sand dune, as opposed to smaller sand ripples or drifts. One dune Curiosity will investigate is as tall as a two-story building and as broad as a football field. The Bagnold Dunes are acti ...
Astronomy Galaxies & The Universe
Astronomy Galaxies & The Universe

... used up → white dwarf (Earth size) Large stars (at least 7 times our sun) when fusion (of carbon) stops, a central iron core is left, intense gravitational energy causes further collapse, creates heavier elements → explosion causes loss of ½ the stars elements, a supernova is born Supernova fades – ...
Two Dissipating Exoplanet Atmospheres Taken from: Hubble
Two Dissipating Exoplanet Atmospheres Taken from: Hubble

... easily lost in the glow of the much brighter stars they circle. Exoplanets were first detected by the small but recognizably cyclic gravitational tug they exert on their stars. Sensitive spectroscopy can measure the tiny changes such a planet induces in its star’s velocity. Once astronomers have est ...
The script - University of Sheffield
The script - University of Sheffield

... picture started out 65 million years ago. What else was happening then? [Children being children, someone will probably know it’s the time at which the dinosaurs became extinct!] Slide 12: The Hubble Ultra-Deep Field Using the Hubble Space Telescope, we can look even further away. Almost everything ...
Chapter 28 Notes
Chapter 28 Notes

... Because of Earth’s movement around the sun Apparent Magnitude – What is it? How bright a star appears to be to an observer on Earth. ...
Astronomy 110 Announcements:
Astronomy 110 Announcements:

... • Kepler first tried to match Tycho’s observations with circular orbits • But an 8 arcminute discrepancy led him eventually to elliptical orbits… “If I had believed that we could ignore these eight minutes [of arc], I would have patched up my hypothesis accordingly. But, since it was not permissible ...
Formation of the Solar System The Solar System
Formation of the Solar System The Solar System

... • Theory that best explains properties of Earth and Moon is “giant impact” between early Earth and a Mars-sized object in a similar orbit. ...
Chapter105.ppt
Chapter105.ppt

... cool and the relationship between star cooling rate and the light they emit or luminosity (star brightness or dimness). • The color of the light emitted by exploding stars in far-off galaxies also provide a measure of distance (“redshift”). ...
Kepler`s Laws and Galileo 8/31/2016
Kepler`s Laws and Galileo 8/31/2016

... relative location of Mars after repeated orbits around the Sun (Mars is close and so most accurate measurements) ...
History of Astronomy
History of Astronomy

... to believe that the Earth was moving. During ancients times, the mathematical and scientific tools were not available to answer the question ...
The Warrumbungle Observer The Warrumbungle Observer
The Warrumbungle Observer The Warrumbungle Observer

... Through a telescope the disc of Jupiter can be easily seen with a pair of parallel brownish stripes. These are cloud bands equivalent to the trade winds on Earth and move in the opposite direction to the spin of the planet. On a night of good seeing, the Great Red Spot can be seen. The Great Red Spo ...
Planets and Stars Key Vocabulary: Comparing and Contrasting
Planets and Stars Key Vocabulary: Comparing and Contrasting

... How can technology be used to observe distant objects in the sky? Technological resources, such as telescopes and space probes, are used to observe distant objects in the sky. Telescopes magnify the appearance of some distant objects in the sky, including the moon and the planets. The number of star ...
Extra-Solar Planets
Extra-Solar Planets

... Planets are plentiful The first planet orbiting another Sun-like star was discovered in 1995. We now know of 209 (Feb 07). Including several stars with more than one planet - true planetary systems ...
Did you know - room11pixies
Did you know - room11pixies

... A black holes is a hole in space that has its own gravitational pull even though they may look black on the outside they are the brightest things in the universe inside. ...
The Small Objects. The Sun.
The Small Objects. The Sun.

The Sun and Other Stars - Tuslaw Local School District
The Sun and Other Stars - Tuslaw Local School District

Scales in the UniverseApollo
Scales in the UniverseApollo

... (diam 1 392 000 km or 109 Earth diameters, distance 150 000 000 km or 1 astronomical unit - 1 AU) ...
ORIGIN OF THE GREEK CONSTELLATIONS
ORIGIN OF THE GREEK CONSTELLATIONS

121mtr
121mtr

... are put on top of older craters; overlapping craters. 11. Explain why the observed retrograde motion of Mars is a problem in the Aristotelian Cosmology and what Ptolemy had to construct to resolve this problem. Answered pretty well but two key words (in bold below) were usually left out  All the pl ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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