1 00:00:05,450 --> 00:00:02,960 a star that wanders too close to a 2 00:00:07,670 --> 00:00:05,460 supermassive black hole is doomed as it 3 00:00:10,280 --> 00:00:07,680 should be ripped apart by extreme tidal 4 00:00:11,839 --> 00:00:10,290 forces the debris from the star is 5 00:00:14,089 --> 00:00:11,849 expected to fall toward the black hole 6 00:00:17,810 --> 00:00:14,099 getting hotter and producing intense 7 00:00:21,560 --> 00:00:17,820 x-rays the x-rays should then fade as 8 00:00:24,019 --> 00:00:21,570 the hot gas spirals inward using Chandra 9 00:00:27,650 --> 00:00:24,029 this behavior may have been spotted for 10 00:00:29,870 --> 00:00:27,660 the first time in a dwarf galaxy bright 11 00:00:33,139 --> 00:00:29,880 x-rays from the location of this small 12 00:00:36,080 --> 00:00:33,149 galaxy were seen in 1999 until they 13 00:00:40,040 --> 00:00:36,090 faded and eventually disappeared in 2005 14 00:00:42,619 --> 00:00:40,050 in the past few years Chandra and other 15 00:00:44,630 --> 00:00:42,629 astronomical satellites have identified 16 00:00:47,360 --> 00:00:44,640 several suspected cases of a 17 00:00:50,060 --> 00:00:47,370 supermassive black hole ripping apart a 18 00:00:52,549 --> 00:00:50,070 nearby star this newly discovered 19 00:00:54,950 --> 00:00:52,559 episode is different because it has been 20 00:00:58,220 --> 00:00:54,960 associated with a much smaller galaxy 21 00:01:00,470 --> 00:00:58,230 than these other cases the black hole 22 00:01:02,660 --> 00:01:00,480 responsible for the destruction may be 23 00:01:05,570 --> 00:01:02,670 only a few hundred thousand times as 24 00:01:07,250 --> 00:01:05,580 massive as the Sun making it 10 times 25 00:01:11,510 --> 00:01:07,260 less massive than the galaxy's 26 00:01:13,190 --> 00:01:11,520 supermassive black hole astronomers 27 00:01:15,649 --> 00:01:13,200 believe that black holes of this size 28 00:01:17,450 --> 00:01:15,659 may be the seeds that ultimately formed