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from gas giants to super
from gas giants to super

... and to the square root of the star luminosities. ...
Volume 20 Number 4 March 2012 - Forsyth Astronomical Society
Volume 20 Number 4 March 2012 - Forsyth Astronomical Society

... fastest winds generated by supermassive black holes, objects millions or billions of times more massive. Also, this is nearly 10 times faster than any seen from a black hole resulting from the collapse of an extremely massive star (stellar-mass black hole). ...
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... Betelgeuse is as large as Saturn's orbit… ...
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Comparing Earth, Sun and Jupiter

... The Sun Mostly Hydrogen and Helium High luminosity due to central fusion reactions Sunspots: cooler regions where magnetic field is strongest More features visible at other wavelengths Types of Stars Characterised mainly by their luminosity and colour Most stars lie on a tight correlation between L ...
The History of Astronomy
The History of Astronomy

... This system explains retrograde motion easily, The Earth was simply passing the by! ...
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... • The current layout of our solar system may bear little resemblance to its original form • This view is more in line with the “planetary migration” thought to occur even more dramatically in many extrasolar planet systems • It may be difficult to prove or disprove these models of our early solar sy ...
The Solar System PPT
The Solar System PPT

... planets because their surfaces are solid (and, as the name implies, somewhat similar to Earth — although the term can be misleading because each of the four has vastly different environments). They’re made up mostly of heavy metals such as iron and nickel, and have either no moons or few moons. ...
Astronomy Assignment #1
Astronomy Assignment #1

... M Star  K  mPlanet  vOrbital mPlanet  ...
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Key 3 - UNLV Physics

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... The orbits of the planets all lie in roughly the same plane The direction they orbit around the Sun is the same as the Sun’s rotation on its axis The direction most planets rotate on their axes is the same as that for the Sun The direction of a planet’s moon orbits is the same as that planet’s direc ...
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... in 1842. This principle is now known as the Doppler effect. He hypothesized that the pitch of a sound would change if the source of the sound were moving. He didn't test this hypothesis until 1845. To test his hypothesis, Doppler used two sets of trumpeters: one set stationary at a train station and ...
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... Group 1 is the four inner planets, and Group 2 is the four outer planets. Group 2 is the six outer planets, and Group 1 is the two inner planets. Group 2 is the two outer planets, and, Group 1 is the six inner planets. Group 1 is the four outer planets, and Group 2 is the four inner planets. ...
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... Comets are thought to originate from a region beyond the orbits of the outermost planets. Scientists believe that gravitational perturbations periodically jar comets out of this population, setting these "dirty snowballs" on orbital courses that bring them closer to the Sun. Some, called long-period ...
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Space Wk 6 Student PPT

... formed as the meteorite is melted by friction as it passes through the atmosphere. • Majority of meteorites that fall are irons- these heavy objects are easier to distinguish from Earth rocks than stony meteorites. • More than 50,000 meteorites found on Earth99.8% come from asteroids ...
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Formation of a Solar System Notes Integrated Science 2 Name: Pd: I

... Surface Evolution continues as a result of ____________________, __________________ and/or ______________________________ ...
< 1 ... 46 47 48 49 50 51 52 53 54 ... 66 >

Astronomical naming conventions

In ancient times, only the Sun and Moon, a few hundred stars and the most easily visible planets had names. Over the last few hundred years, the number of identified astronomical objects has risen from hundreds to over a billion, and more are discovered every year. Astronomers need to be able to assign systematic designations to unambiguously identify all of these objects, and at the same time give names to the most interesting objects and, where relevant, features of those objects.The International Astronomical Union (IAU) is the officially recognized authority in astronomy for assigning designations to celestial bodies such as stars, planets, and minor planets, including any surface features on them. In response to the need for unambiguous names for astronomical objects, it has created a number of systematic naming systems for objects of various sorts.
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