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Clues to the Origin of the Solar System
Clues to the Origin of the Solar System

... ! Sun, Jupiter, and Saturn have same hydrogen dominated composition implying they formed from the same materials. ! Terrestrial planets and satellites are deficient in light gases and ices. Formed too close to Sun for gases/ices to remain, leaving heavier rock and metal. ...
Ancient astronomy Part 8
Ancient astronomy Part 8

... Many ancient North American tribes were hunter-gatherers who developed their astronomy in a context which differed from the mostly settled agricultural civilisations in Europe. They also commonly believe in a oneness with all life, all living things, including celestial objects, being inter-related. ...
ExoplanetWorksheet
ExoplanetWorksheet

... *All of the rocky planets in our Solar System are at least 3 times more dense than Jupiter. Does it look like we’ve found very many or very few rocky exoplanets? __________________________________ * White dwarf stars have a mass that is comparable to the Sun, but are about 100 times smaller. Have we ...
Meteors - Little Worksheets
Meteors - Little Worksheets

... The correct name for a shooting star is meteor. Besides very large objects like stars, planets and moons, space has lots of little objects. These can be rocks in space left over from old planets. These objects can even be as small as a speck of dust. These objects are called meteorites. When a meteo ...
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Astronomy PowerPoint - Petal School District
Astronomy PowerPoint - Petal School District

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The Sun, the closest star - University of Iowa Astrophysics
The Sun, the closest star - University of Iowa Astrophysics

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Section 14.7: The Sun

...  Its gravitational pull keeps us in our steady orbit  1.4 million km across (the earth is only 13000 km across)  To compare sizes, if the Sun is a basketball, the Earth would be the head of a pin ...
Ch16: The Milky Way
Ch16: The Milky Way

HW4 due - Yale Astronomy
HW4 due - Yale Astronomy

... to  be  0.005  arcsecond?  Express  your  answer  in  both  light  years  and  parsecs.   ...
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Word doc - UC-HiPACC - University of California, Santa Cruz

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ppt - Serbian Virtual Observatory - astronomical observatory belgrade

PHYS 200 - Understanding the Universe
PHYS 200 - Understanding the Universe

... • grasp how physical principles are applied to understand cosmic objects. • Gain appreciation for science and scientific methods and to realize that progress in the understanding of the Universe is achieved by continual questioning of current knowledge. • Report on: what makes up the solar system, w ...
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... Star + planet orbit about centre of gravity We can also see the motion of the star from its spectral lines. ...
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Name ______KEY Date Core ______ Study Guide Galaxies and the

... Why can’t we see all of the Milky Way from Earth? The Earth is inside the disk of the Milky Way so we only have an edge view and can only view part of it. You can’t see the center of the galaxy because it’s hidden by the dust – also, we can only see a small fraction of the stars because of they’re t ...
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changing constellations

... So, what is going on? The ause each day bec r yea the ing change dur n 2.5 million the Earth moves more tha the Sun (or und aro kilometres as it orbits stars The it). orb full a about 1/365th of dually gra ht nig mid at ds hea above our g a full cycle in change each night, makin one year. kes an ext ...
Astronomy 114 Problem Set # 7 Due: 30 Apr 2007 SOLUTIONS 1
Astronomy 114 Problem Set # 7 Due: 30 Apr 2007 SOLUTIONS 1

... a fraction of an arc second at best. Especially for ground-based telescopes, the main goal is collecting photons! 2 How big would a radio telescope observing at 20 cm wavelength have to be in order to resolve the same angle as the Keck telescope in the last problem? Since 20 cm is in radio wavelengt ...
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688 Chapter 21 Review - District 196 e

... 3.8 × 1026 watts and the distance between the sun and Earth is 150 × 109 meters. b. Suppose Earth were orbiting Alpha Centaurii A, the nearest star to Earth. This star has a luminosity of 5.7 × 1026 watts. Calculate the intensity of light at Earth’s orbit around Alpha Centaurii A and discuss whether ...
Space Unit - Questions and Answers
Space Unit - Questions and Answers

... A solar prominence is a burst of a huge sheet of gases, also from the inner atmosphere. It is much larger than a flare and may last for days or even weeks. The charged particles from a solar flare affect us in two main ways: They produce the beautiful auroras, and they cause problems in communicatio ...
Wednesday - Syracuse University
Wednesday - Syracuse University

... lightyear is the distance light travels in one year. It is equal to 9.46 × 1012 km. The 11th closest star to our solar system is Epsilon Eridani. It is 3.22 parsecs away. What is its distance from the sun in meters and how many seconds does its light take to get to us? ...
ASTR101
ASTR101

... • Theory fits our system well • Need to look at other planetary  systems to see if we are common or  unusual ...
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... today and other stars that are ten billion years old, so unlike the planets of the Solar System, which can only be observed as they are today, studying exoplanets allows the observation of exoplanets at different stages of evolution. • When planets form they have hydrogen envelopes that cool and con ...
From Big bang to lives on planets
From Big bang to lives on planets

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R136a1



RMC 136a1 (usually abbreviated to R136a1) is a Wolf-Rayet star located at the center of R136, the central condensation of stars of the large NGC 2070 open cluster in the Tarantula Nebula. It lies at a distance of about 50 kiloparsecs (163,000 light-years) in the Large Magellanic Cloud. It has the highest mass and luminosity of any known star, at 265 M☉ and 8.7 million L☉, and also one of the hottest at over 50,000 K.
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