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Nineteenth lecture
Nineteenth lecture

The Sun, at a mean distance of 92.96 million miles, is the closest
The Sun, at a mean distance of 92.96 million miles, is the closest

... huge sphere of mostly ionized gas, supports all life on Earth. It powers photosynthesis in green plants, and is ultimately the source of all food and energy. In fact, the Sun produces in 1 second the U.S. energy needs for 90,000 years! The connection and interactions between the Sun and Earth drive ...
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... 23. What category of star is Sirius B? 24. Which giant is the brightest? 25. Predict what will happen when the sun runs out of fuel. 26. What is used to classify stars? 27. At which phase of the moon could a solar eclipse occur? 28. A star is twice as massive as the sun. How will its lifespan compa ...
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Today`s Powerpoint

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...  Main Sequence Stars -- make up the majority of stars in the universe. Earth’s sun is a main sequence star. These stars vary in size, mass, and brightness, but they all convert hydrogen into helium, also known as nuclear fusion. While our sun will spend 10 billion on its main sequence, a star ten t ...
Celestial Bodies
Celestial Bodies

< 1 ... 108 109 110 111 112 113 114 115 116 118 >

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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