๐Ÿš€ ๅฎ‡ๅฎ™ใฎ่จ˜ๆ†ถใƒปใ‚ซใƒฌใƒณใƒ€ใƒผๆคœ็ดข
ใใ‚‡ใ† ใƒฉใƒณใƒ€ใƒ 
CTB 1: ้ซ„่ณชๆ˜Ÿ้›ฒ CTB 1: The Medulla Nebula
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ใ“ใฎ็ใ—ใ„ๆ˜Ÿ้›ฒใฎใ‚จใƒใƒซใ‚ฎใƒผๆบใฏไฝ•ใงใ—ใ‚‡ใ†ใ‹? CTB 1 ใฏใ€็ด„ 1 ไธ‡ๅนดๅ‰ใ€ใ‚ซใ‚ทใ‚ชใƒšใƒคๅบงใฎๆ–นๅ‘ใซใ‚ใ‚‹ๅทจๅคงใชๆ’ๆ˜ŸใŒ็ˆ†็™บใ—ใŸใจใใซๆฎ‹ใฃใŸ่†จๅผตใ‚ฌใ‚นๆฎปใงใ™ใ€‚ใ“ใฎๆ’ๆ˜Ÿใฏใ€ๆ ธ่žๅˆๅๅฟœใงๅฎ‰ๅฎšๅœงๅŠ›ใ‚’็”Ÿๆˆใงใใ‚‹ๅ…ƒ็ด ใŒไธญๅฟƒๆ ธ่ฟ‘ใใงๆžฏๆธ‡ใ—ใŸใŸใ‚ใซ็ˆ†็™บใ—ใŸใจ่€ƒใˆใ‚‰ใ‚Œใพใ™ใ€‚ใใฎ็ตๆžœใงใใŸ่ถ…ๆ–ฐๆ˜Ÿๆฎ‹้ชธใฏใ€่„ณใฎใ‚ˆใ†ใชๅฝขใ‚’ใ—ใฆใ„ใ‚‹ใ“ใจใ‹ใ‚‰ใƒกใƒ‡ใƒฅใƒฉๆ˜Ÿ้›ฒใจใ„ใ†ๆ„›็งฐใงๅ‘ผใฐใ‚Œใ€้–‰ใ˜่พผใ‚ใ‚‰ใ‚Œใฆใ„ใ‚‹ๆ˜Ÿ้–“ใ‚ฌใ‚นใจใฎ่ก็ชใง็™บ็”Ÿใ—ใŸ็†ฑใฎใŸใ‚ใ€ไปŠใ‚‚ๅฏ่ฆ–ๅ…‰ใง่ผใ„ใฆใ„ใพใ™ใ€‚ใ—ใ‹ใ—ใ€ใชใœใ“ใฎๆ˜Ÿ้›ฒใŒ X ็ทšใงใ‚‚่ผใใฎใ‹ใฏใ€ใพใ ็ ”็ฉถไธญใงใ™ใ€‚1 ใคใฎไปฎ่ชฌใงใฏใ€ๅผทๅŠ›ใชใƒ‘ใƒซใ‚ตใƒผใŒ็”Ÿๆˆใ•ใ‚Œใ€ๅค–ๅ‘ใใซ้ซ˜้€Ÿใง็งปๅ‹•ใ™ใ‚‹้ขจใงๆ˜Ÿ้›ฒใฎใ‚จใƒใƒซใ‚ฎใƒผใ‚’ไพ›็ตฆใ—ใฆใ„ใ‚‹ใจ่€ƒใˆใ‚‰ใ‚Œใฆใ„ใพใ™ใ€‚ใ“ใฎๆ‰‹ใŒใ‹ใ‚Šใ‚’ใŸใฉใ‚Šใ€่ถ…ๆ–ฐๆ˜Ÿ็ˆ†็™บใซใ‚ˆใฃใฆ็ง’้€Ÿ 1,000 ใ‚ญใƒญใƒกใƒผใƒˆใƒซใ‚’่ถ…ใˆใ‚‹้€Ÿๅบฆใงๆ”พๅ‡บใ•ใ‚ŒใŸใจๆ€ใ‚ใ‚Œใ‚‹ใƒ‘ใƒซใ‚ตใƒผใŒ้›ปๆณขใง็™บ่ฆ‹ใ•ใ‚Œใพใ—ใŸใ€‚ใƒกใƒ‡ใƒฅใƒฉๆ˜Ÿ้›ฒใฏๆบ€ๆœˆใจๅŒใ˜ใใ‚‰ใ„ใฎๅคงใใ•ใซ่ฆ‹ใˆใพใ™ใŒใ€้žๅธธใซๆš—ใ„ใŸใ‚ใ€ใ“ใฎ็”ปๅƒใ‚’ไฝœๆˆใ™ใ‚‹ใŸใ‚ใซใ€็ฑณๅ›ฝใƒ†ใ‚ญใ‚ตใ‚นๅทžใฎๅฐๅž‹ๆœ›้ ้กใง 84 ๆ™‚้–“ใฎ้œฒๅ‡บใ‚’่ฆใ—ใพใ—ใŸใ€‚
ๅŽŸๆ–‡๏ผˆEnglish๏ผ‰
What powers this unusual nebula? CTB 1 is the expanding gas shell that was left when a massive star toward the constellation of Cassiopeia exploded about 10,000 years ago. The star likely detonated when it ran out of elements, near its core, that could create stabilizing pressure with nuclear fusion. The resulting supernova remnant, nicknamed the Medulla Nebula for its brain-like shape, still glows in visible light because of the heat generated by its collision with confining interstellar gas. Why the nebula also glows in X-ray light, though, remains a topic of research. One hypothesis holds that an energetic pulsar was created and powers the nebula with a fast outwardly moving wind. Following this lead, a pulsar was found in radio waves that appears to have been expelled by the supernova explosion at over 1000 kilometers per second. Although the Medulla Nebula appears as large as a full moon, it is so faint that it took 84-hours of exposure with a small telescope in Texas, USA, to create the featured image.

๏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