็ฝ่ฒ็ฎๆใฏใใฃใใใ
White Dwarfs Cool
ไธใฎๅ็ใงไธธใงๅฒใพใใๆใ
ใฏใๅฎๅฎใงใฏ่ฆใคใใใฎใ้ฃใใ็ฝ่ฒ็ฎๆใฎไธ็จฎใงใใใใฎๅ็ใฏใM4ใจๅผใฐใใ็็ถๆๅฃใฎไธญๅฟไป่ฟใฎๅฐใใช้ ๅใๆใใใใฎใงใใใใใใซๅฎๅฎๆ้ ้กใ็จใใ็ ็ฉถ่
ใใกใฏใM4ใซ็ฝ่ฒ็ฎๆใๅฏ้ใใฆใใใใจใ็บ่ฆใใพใใใใใใฏไบๆณใใใฆใใใใจใงใๅคช้ฝใๅซใไฝ่ณช้ๆใฏ็ฝ่ฒ็ฎๆใธใจ้ฒๅใใใใจใ็ฅใใใฆใใพใใ็ฝ่ฒ็ฎๆใฏ้ๅธธใใไปฅไธ้ฒๅใใใ้ซๆธฉใใๅพใ
ใซๅทใใฆใใใพใใใใใใฎๆใใฉใฎใใใซๅทใใฆใใใใ็ ็ฉถใใใใจใงใๆใฎๅนด้ฝขใ่ฆชๆๅฃใฎๅนด้ฝขใใใใฆใฒใใฆใฏๅฎๅฎใฎๅนด้ฝขใพใงใใใๆทฑใ็่งฃใงใใใจๆๅพ
ใใใฆใใพใใ
ๅๆ๏ผEnglish๏ผ
The circled stars in the above picture are from a class that is hard to see in the cosmos: white dwarfs. The entire photo covers a small region near the center of a globular cluster known as M4. Researchers using the Hubble Space Telescope discovered a large concentration of white dwarfs in M4. This was expected - low mass stars, including the Sun, are known to evolved to the white dwarf stage. White dwarfs do not usually evolve further, they just gradually cool down from their high temperatures. It is hoped that studying how these stars cool could lead to a better understanding of their ages, of the age of their parent globular cluster, and hopefully even the age of our universe!
๏ผผ ใใฎๆๅใๅฎๅฎไปฒ้ใซใทใงใข ๏ผ
ๅฎๅฎใXใงใทใงใข
ยฉ NASA / APOD