M105 (aka NGC 3379) - Hubble peered into the core of M105 (also known as NGC 3379) and measured the motions of stars swirling around its center. These observations proved that a supermassive black hole resides at the galaxy’s heart. According to recent estimates, this black hole could be up to 200 million times as massive as our Sun. Credits: NASA, ESA, Karl Gebhardt (University of Michigan) and Tod Lauer (NOAO)
M105 is an elliptical galaxy 32 billion light-years away in the constellation Leo. It is the largest elliptical in the Messier catalog that is not a member of the Virgo cluster of galaxies. M105 does, however, belong to the M96 (or Leo I) Group, which includes neighbors M95 and M96 as well as several other fainter galaxies. Charles Messier’s colleague Pierre Méchain discovered M105 in 1781 just a few days after locating M95 and M96. Yet M105 was not originally included in Messier’s catalog. It was added in 1947 after astronomer Helen S. Hogg found a letter written by Méchain describing the galaxy.
This Hubble image of M105 was taken in near-infrared and visible light. Like most elliptical galaxies it appears rather featureless and inactive. However, Hubble observations surprised astronomers by revealing young stars and star clusters in M105, indicating that star formation is still taking place in what was thought to be a “dead” galaxy no longer capable of giving birth to new stars. Other Hubble observations measured the speeds of stars moving around the center of the galaxy, which demonstrated that a supermassive black hole resides at M105’s core.
Best observed in April, M105 has an apparent magnitude of 10.2 and can be spotted with a small telescope. Large telescopes will uncover two fainter galaxies (NGC 3384 and NGC 3389) close to the bright elliptical.
For more information about Hubble’s observations of M105, see:
Credits: NASA, ESA, STScI and C. Sarazin (University of Virginia)
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This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or . For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
{{Information |Description=Messier 105 M105 (aka NGC 3379) - Hubble peered into the core of M105 (also known as NGC 3379) and measured the motions of stars swirling around its center. These observations proved that a supermassive black hole resides at...
ไฟล, m105, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลาง, อม, ลเก, ยวก, บภาพขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, โลไบต, ชน, ดไมม, image, jpeg, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอย, คอมมอนส, ราย. ifl prawtiifl hnathimiphaphni karichiflswnklang khxmulekiywkbphaphkhnadkhxngtwxyangni 600 600 phikesl khwamlaexiydxun 240 240 phikesl 480 480 phikesl 985 985 phikesl duphaphthimikhwamlaexiydsungkwa 8206 985 985 phikesl khnadifl 38 kiolibt chnidimm image jpeg rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khaxthibayM105 jpg Messier 105M105 aka NGC 3379 Hubble peered into the core of M105 also known as NGC 3379 and measured the motions of stars swirling around its center These observations proved that a supermassive black hole resides at the galaxy s heart According to recent estimates this black hole could be up to 200 million times as massive as our Sun Credits NASA ESA Karl Gebhardt University of Michigan and Tod Lauer NOAO M105 is an elliptical galaxy 32 billion light years away in the constellation Leo It is the largest elliptical in the Messier catalog that is not a member of the Virgo cluster of galaxies M105 does however belong to the M96 or Leo I Group which includes neighbors M95 and M96 as well as several other fainter galaxies Charles Messier s colleague Pierre Mechain discovered M105 in 1781 just a few days after locating M95 and M96 Yet M105 was not originally included in Messier s catalog It was added in 1947 after astronomer Helen S Hogg found a letter written by Mechain describing the galaxy This Hubble image of M105 was taken in near infrared and visible light Like most elliptical galaxies it appears rather featureless and inactive However Hubble observations surprised astronomers by revealing young stars and star clusters in M105 indicating that star formation is still taking place in what was thought to be a dead galaxy no longer capable of giving birth to new stars Other Hubble observations measured the speeds of stars moving around the center of the galaxy which demonstrated that a supermassive black hole resides at M105 s core Best observed in April M105 has an apparent magnitude of 10 2 and can be spotted with a small telescope Large telescopes will uncover two fainter galaxies NGC 3384 and NGC 3389 close to the bright elliptical For more information about Hubble s observations of M105 see http hubblesite org news release news 1997 01aehlngthima https www nasa gov feature goddard 2017 messier 105phusrangsrrkh Credits NASA ESA STScI and C Sarazin University of Virginia karxnuyat karichiflniihm Public domain Public domain false falseThis file is in the public domain because it was created by NASA and ESA NASA Hubble material and ESA Hubble material prior to 2009 is copyright free and may be freely used as in the public domain without fee on the condition that only NASA STScI and or ESA is credited as the source of the material This license does not apply if ESA material created after 2008 or source material from other organizations is in use The material was created for NASA by Space Telescope Science Institute under Contract NAS5 26555 or for ESA by the Hubble European Space Agency Information Centre Copyright statement at hubblesite org or 2008 copyright statement at spacetelescope org For material created by the European Space Agency on the spacetelescope org site since 2009 use the ESA Hubble tag prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn21 37 22 tulakhm 2560985 985 38 kiolibt Fabian RRRR Information Description Messier 105 M105 aka NGC 3379 Hubble peered into the core of M105 also known as NGC 3379 and measured the motions of stars swirling around its center These observations proved that a supermassive black hole resides at hnathimiphaphni hnatxipni oyngmathiphaphni raychuxwtthuthxngfakhxngemsiey karichiflswnklang wikixuntxipniichiflni karichbn de wikipedia org Messier Katalog karichbn pl wikipedia org Messier 105 karichbn ru wikipedia org M 105 galaktika karichbn sv wikipedia org Messier 105khxmulekiywkbphaph phaphnimikhxmulephimetim sungswnihymacakklxngdicitxlhruxsaeknenxrthisamarthekbkhxmuldngklawiwrwmkbphaphid thaphaphnithukprbprungaekikhhruxepliynaeplngcakedim khxmulbangxyangcayngkhngimepliynaeplngehmuxnphaphthithukprbprungaekikhnnkarcdwangphaphpktikhwamlaexiydaenwnxn72 dpikhwamlaexiydaenwtng72 dpisxftaewrthiichAdobe Photoshop CC 2017 Windows aekikhphaphlasud11 25 5 tulakhm 2560sepssiimidprbethiybewlathiaeplngepndicithl07 19 5 tulakhm 2560wnthiaekikhkhxmulemtalasud07 25 5 tulakhm 2560ID echphaakhxngexksartnchbbxmp did d4245b5b a9e2 1a40 a3d5 c0cb5d85c390 ekhathungcak https th wikipedia org wiki ifl M105 jpg, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
