1 00:00:00,020 --> 00:00:04,040 [No Audio] 2 00:00:12,100 --> 00:00:08,090 [Bwaaam] 3 00:00:12,120 --> 00:00:16,130 [Bwaam] When we started watching it, we 4 00:00:16,150 --> 00:00:20,170 had no idea how dynamic this system was. [Music] 5 00:00:20,190 --> 00:00:24,180 [Music] 6 00:00:24,200 --> 00:00:28,230 We still don't know what it's capable of. [Whoosh] 7 00:00:28,250 --> 00:00:32,260 [Bwaaam] The only way these readings make 8 00:00:32,280 --> 00:00:36,320 sense is if this pulsar is orbiting a star. 9 00:00:36,340 --> 00:00:40,320 We've never seen one in an orbit this long. The binary 10 00:00:40,340 --> 00:00:44,340 companion is one of the brightest stars in our galaxy, and the pulsar is going to 11 00:00:44,360 --> 00:00:48,410 pass incredibly close to it! This pulsar has been 12 00:00:48,430 --> 00:00:52,430 accelerating for the last ten years, and it's still speeding up. 13 00:00:52,450 --> 00:00:56,520 [Bwaam] 14 00:00:56,540 --> 00:01:00,550 When it passes through the companion star's disk, we're gonna see some serious 15 00:01:00,570 --> 00:01:04,600 gamma-ray emission. Fermi will be watching in 16 00:01:04,620 --> 00:01:08,660 gamma rays. It has the tools. 17 00:01:16,760 --> 00:01:12,710 [Music] 18 00:01:16,780 --> 00:01:20,820 There's so much we can learn from this. 19 00:01:20,840 --> 00:01:24,860 [Music] 20 00:01:24,880 --> 00:01:28,880 [Wwraum] 21 00:01:28,900 --> 00:01:32,920 We're going to need a bigger hard drive 22 00:01:32,940 --> 00:01:36,990 [Wwraum] [indistinct radio voices] 23 00:01:37,010 --> 00:01:41,030 [indistinct radio voices]