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Here are the 20 hottest female celebrities in the industry. Jessica Biel Jessica Biel is fit, hot, and talented. Jennifer Lawrence Jennifer Lawrence is a superstar—and one of the most beautiful women in Hollywood.
Kendra Wilkinson. And she's got a real talent for rodeo. Kim Kardashian. Paris Hilton. In other words, she got famous from a guy doing her on camera.
She and Kim were also friends once! This Earth-sized sphere, consisting mainly of carbon and oxygen, is incredibly dense, the most massive up to around 1.
Only something called electron degeneracy pressure, an outward pressure generated by the inability of electrons with the same spin to occupy the same state, prevents the core from complete collapse.
Because they are so dense, with such a small surface area, they take a very long time to lose heat.
Once the core of a white dwarf has stopped contracting, it can exceed temperatures of around , Kelvin around , degrees Celsius and , degrees Fahrenheit.
Astronomers think that not enough time has passed since the beginning of the Universe for a white dwarf to have cooled completely.
But the so-called Q-branch white dwarf stars, which constitute around 6 percent of massive white dwarfs, cool even slower than that. According to a paper led by astronomer Sihao Cheng of Johns Hopkins University, this small fraction of white dwarfs demonstrate a cooling delay of about 8 billion years, compared to other white dwarfs.
Some stars shine more brightly than others. Their brightness is a factor of how much energy they put out—known as luminosity —and how far away from Earth they are.
Color can also vary from star to star because their temperatures are not all the same. Hot stars appear white or blue, whereas cooler stars appear to have orange or red hues.
By plotting these and other variables on a graph called the Hertzsprung-Russell diagram, astronomers can classify stars into groups.
Along with main sequence and white dwarf stars, other groups include dwarfs, giants, and supergiants. Supergiants may have radii a thousand times larger than that of our own sun.
Stars spend 90 percent of their lives in their main sequence phase. Now around 4. As stars move toward the ends of their lives, much of their hydrogen has been converted to helium.
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