๐Ÿš€ ๅฎ‡ๅฎ™ใฎ่จ˜ๆ†ถใƒปใ‚ซใƒฌใƒณใƒ€ใƒผๆคœ็ดข
ใใ‚‡ใ† ใƒฉใƒณใƒ€ใƒ 
GL 229B: ่ฌŽใฎ่ค่‰ฒ็Ÿฎๆ˜Ÿ? GL 229B: An Elusive Brown Dwarf?
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ๅฎ‡ๅฎ™ใฎๅคง้ƒจๅˆ†ใฏใฉใฎใ‚ˆใ†ใช็‰ฉ่ณชใงๆง‹ๆˆใ•ใ‚Œใฆใ„ใ‚‹ใฎใงใ—ใ‚‡ใ†ใ‹๏ผŸใ“ใฎๅ•ใ„ใฏใ€็พไปฃใฎๅคฉๆ–‡ๅญฆใซใŠใ‘ใ‚‹ๆœ€ใ‚‚้›ฃ่งฃใช่ฌŽใจ่จ€ใˆใ‚‹ใงใ—ใ‚‡ใ†ใ€‚ๆœ‰ๅŠ›ใชๅ€™่ฃœใฎไธ€ใคใฏใ€ใ€Œ่ค่‰ฒ็Ÿฎๆ˜Ÿใ€ใจๅ‘ผใฐใ‚Œใ‚‹ใ€ๆš—ใ่ณช้‡ใฎๅฐใ•ใ„ๆ˜Ÿใงใ™ใ€‚็งใŸใกใฎๅฎ‡ๅฎ™ใซใฏใ€ไป–ใฎใฉใฎ็จฎ้กžใฎๆ˜Ÿใ‚ˆใ‚Šใ‚‚ๅคšใใฎ่ค่‰ฒ็Ÿฎๆ˜ŸใŒๅญ˜ๅœจใ™ใ‚‹ๅฏ่ƒฝๆ€งใŒใ‚ใ‚Šใพใ™ใŒใ€ใใ‚Œใ‚‰ใฏ้žๅธธใซๆš—ใ„ใŸใ‚ใ€ใ“ใ‚Œใพใง็™บ่ฆ‹ใ•ใ‚Œใฆใ„ใพใ›ใ‚“ใ€‚1994ๅนด10ๆœˆใซๆ’ฎๅฝฑใ•ใ‚ŒใŸไธŠใฎใƒ‰ใƒฉใƒžใƒใƒƒใ‚ฏใชๅ†™็œŸใฏใ€ใ“ใฎใ€Œๆš—้ป’็‰ฉ่ณชใ€ๅ•้กŒใซๆ–ฐใŸใชๅ…‰ใ‚’ๅฝ“ใฆใฆใ„ใพใ™ใ€‚้œฒๅ‡บใ‚ชใƒผใƒใƒผใง้€šๅธธใฎๆ˜Ÿใฎๅณๅดใซ่ฆ‹ใˆใ‚‹ใ€ไธ€่ฆ‹็›ฎ็ซ‹ใŸใชใ„ไผดๆ˜Ÿใฏใ€ๆ‰ใˆใฉใ“ใ‚ใฎใชใ„่ค่‰ฒ็Ÿฎๆ˜Ÿใงใ‚ใ‚‹ใจ่€ƒใˆใ‚‰ใ‚Œใฆใ„ใพใ™ใ€‚่ค่‰ฒ็Ÿฎๆ˜Ÿใฎๅญ˜ๅœจใŒๅฎŸ่จผใ•ใ‚ŒใŸไปŠใ€ๆฎ‹ใ•ใ‚ŒใŸ้‡่ฆใช็–‘ๅ•ใฏใ€ใใฎๅญ˜ๅœจ้‡ใงใ™ใ€‚
ๅŽŸๆ–‡๏ผˆEnglish๏ผ‰
What type of matter makes up most of the universe? This question is arguably the most perplexing astronomical mystery of our time. A leading candidate is a type of dim, low mass star called a "brown dwarf" star. Our universe could contain more brown dwarfs than any other type of star - but they are so dim they have so far escaped detection. The dramatic photograph above, taken in October 1994, sheds new light on this "dark matter" problem. The seemingly inconspicuous companion to the right of the overexposed image of a normal star is thought to be an elusive brown dwarf. Now that the existence of brown dwarfs has been demonstrated, a key remaining question is their abundance.

๏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