๐Ÿš€ ๅฎ‡ๅฎ™ใฎ่จ˜ๆ†ถใƒปใ‚ซใƒฌใƒณใƒ€ใƒผๆคœ็ดข
ใใ‚‡ใ† ใƒฉใƒณใƒ€ใƒ 
็™ฝ่‰ฒ็Ÿฎๆ˜Ÿใฏใ‹ใฃใ“ใ„ใ„ White Dwarfs Cool
โœ… Public Domain
ไธŠใฎๅ†™็œŸใงไธธใงๅ›ฒใพใ‚ŒใŸๆ˜Ÿใ€…ใฏใ€ๅฎ‡ๅฎ™ใงใฏ่ฆ‹ใคใ‘ใ‚‹ใฎใŒ้›ฃใ—ใ„็™ฝ่‰ฒ็Ÿฎๆ˜Ÿใฎไธ€็จฎใงใ™ใ€‚ใ“ใฎๅ†™็œŸใฏใ€M4ใจๅ‘ผใฐใ‚Œใ‚‹็ƒ็Šถๆ˜Ÿๅ›ฃใฎไธญๅฟƒไป˜่ฟ‘ใฎๅฐใ•ใช้ ˜ๅŸŸใ‚’ๆ‰ใˆใŸใ‚‚ใฎใงใ™ใ€‚ใƒใƒƒใƒ–ใƒซๅฎ‡ๅฎ™ๆœ›้ ้กใ‚’็”จใ„ใŸ็ ”็ฉถ่€…ใŸใกใฏใ€M4ใซ็™ฝ่‰ฒ็Ÿฎๆ˜ŸใŒๅฏ†้›†ใ—ใฆใ„ใ‚‹ใ“ใจใ‚’็™บ่ฆ‹ใ—ใพใ—ใŸใ€‚ใ“ใ‚Œใฏไบˆๆƒณใ•ใ‚Œใฆใ„ใŸใ“ใจใงใ€ๅคช้™ฝใ‚’ๅซใ‚€ไฝŽ่ณช้‡ๆ˜Ÿใฏ็™ฝ่‰ฒ็Ÿฎๆ˜Ÿใธใจ้€ฒๅŒ–ใ™ใ‚‹ใ“ใจใŒ็Ÿฅใ‚‰ใ‚Œใฆใ„ใพใ™ใ€‚็™ฝ่‰ฒ็Ÿฎๆ˜Ÿใฏ้€šๅธธใใ‚ŒไปฅไธŠ้€ฒๅŒ–ใ›ใšใ€้ซ˜ๆธฉใ‹ใ‚‰ๅพใ€…ใซๅ†ทใˆใฆใ„ใใพใ™ใ€‚ใ“ใ‚Œใ‚‰ใฎๆ˜ŸใŒใฉใฎใ‚ˆใ†ใซๅ†ทใˆใฆใ„ใใ‹ใ‚’็ ”็ฉถใ™ใ‚‹ใ“ใจใงใ€ๆ˜Ÿใฎๅนด้ฝขใ€่ฆชๆ˜Ÿๅ›ฃใฎๅนด้ฝขใ€ใใ—ใฆใฒใ„ใฆใฏๅฎ‡ๅฎ™ใฎๅนด้ฝขใพใงใ‚‚ใ‚ˆใ‚Šๆทฑใ็†่งฃใงใใ‚‹ใจๆœŸๅพ…ใ•ใ‚Œใฆใ„ใพใ™ใ€‚
ๅŽŸๆ–‡๏ผˆEnglish๏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 ใ“ใฎๆ„Ÿๅ‹•ใ‚’ๅฎ‡ๅฎ™ไปฒ้–“ใซใ‚ทใ‚งใ‚ข ๏ผ

ๅฎ‡ๅฎ™ใ‚’Xใงใ‚ทใ‚งใ‚ข
ยฉ NASA / APOD