MAXI J1659-152: Difference between revisions
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MAXI J1659-152 is a rapidly rotating [[black-hole]]/star system, discovered by [[NASA]]’s Swift space telescope on 25 September 2010. On March the 19th 2013 [[ESA]]’s XMM-Newton space telescope has helped to identify a star and a black hole that orbit each other at the dizzying rate of once every 2.4 hours. |
MAXI J1659-152 is a rapidly rotating [[black-hole]]/star system, discovered by [[NASA]]’s Swift space telescope on 25 September 2010. On March the 19th 2013 [[ESA]]’s XMM-Newton space telescope has helped to identify a star and a black hole that orbit each other at the dizzying rate of once every 2.4 hours. |
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The black hole and the [[star]] orbit their common center of mass. Because the star is the lighter object, it lies further from this point and has to travel around its larger [[orbit]] at a breakneck speed of two million kilometers per hour |
The black hole and the [[star]] orbit their common center of mass. Because the star is the lighter object, it lies further from this point and has to travel around its larger [[orbit]] at a breakneck speed of two million kilometers per hour, which is 555 kilometers per second. The star is the fastest moving star ever seen in an X-ray [[binary system]]. <br/>On the other hand, the black hole orbits at ‘only’ 150 000 km/h. |
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The black hole in this compact pairing is at least three times more massive than the [[Sun]], while its [[red dwarf]] companion star has a [[mass]] only 20% that of the Sun. The pair is separated by roughly a million kilometers.<ref>[http://www.esa.int/Our_Activities/Space_Science/Black_hole-star_pair_orbiting_at_dizzying_speed MAXI J1659-152: The shortest orbital period black-hole transient in outburst (2012)]</ref> |
The black hole in this compact pairing is at least three times more massive than the [[Sun]], while its [[red dwarf]] companion star has a [[mass]] only 20% that of the Sun. The pair is separated by roughly a million kilometers - for comparison the distance to the Sun from Earth is about 150 million kilometers.<ref>[http://www.esa.int/Our_Activities/Space_Science/Black_hole-star_pair_orbiting_at_dizzying_speed MAXI J1659-152: The shortest orbital period black-hole transient in outburst (2012)]</ref> |
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==References== |
==References== |
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Revision as of 08:49, 28 March 2013
MAXI J1659-152 is a rapidly rotating black-hole/star system, discovered by NASA’s Swift space telescope on 25 September 2010. On March the 19th 2013 ESA’s XMM-Newton space telescope has helped to identify a star and a black hole that orbit each other at the dizzying rate of once every 2.4 hours.
The black hole and the star orbit their common center of mass. Because the star is the lighter object, it lies further from this point and has to travel around its larger orbit at a breakneck speed of two million kilometers per hour, which is 555 kilometers per second. The star is the fastest moving star ever seen in an X-ray binary system.
On the other hand, the black hole orbits at ‘only’ 150 000 km/h.
The black hole in this compact pairing is at least three times more massive than the Sun, while its red dwarf companion star has a mass only 20% that of the Sun. The pair is separated by roughly a million kilometers - for comparison the distance to the Sun from Earth is about 150 million kilometers.[1]