1 00:00:00,990 --> 00:00:07,620 \h The Chandra X-ray Observatory orbits high above the Earth, peering into the blackest reaches of space. 2 00:00:07,620 --> 00:00:13,200 \h Exploring the most menacing and magnificent features of the cosmos, this remarkable telescope is 3 00:00:13,200 --> 00:00:30,880 \h revealing what our eyes can't, taking us beyond visible light. 4 00:00:30,880 --> 00:00:38,260 \h NARRATOR: The cosmic ocean twinkles and transforms with the birth of stars and their explosive demise into supernovas. 5 00:00:38,260 --> 00:00:45,490 \h Brilliantly bright and wrought with destructive power, supernovas and their gaseous remnants are a frequent target of NASA's 6 00:00:45,490 --> 00:00:53,540 \h Chandra X-ray Observatory because of the clues they give us about their earlier lives as stars. 7 00:00:53,540 --> 00:01:00,330 \h Equipped with X-ray detectors to cut through the clutter and glare that blind optical telescopes, 8 00:01:00,330 --> 00:01:07,320 \h Chandra's revealed details about supernovas that help to shown them for the stars that they once were. 9 00:01:07,320 --> 00:01:13,820 \h DR. PAT SLANE: You see the effects of the swept-up interstellar medium lighting up a ring of X-ray emission. 10 00:01:13,820 --> 00:01:20,800 \h You see the effects of the back pressure from that, pushing back toward the inside of the explosion where all the ejecta, 11 00:01:20,800 --> 00:01:27,160 \h the stuff that was formed in the explosion in the interior of the star, flying out. 12 00:01:27,160 --> 00:01:31,510 \h That's being compressed and heated to X-ray temperatures, as well. 13 00:01:31,510 --> 00:01:36,270 \h NARRATOR: Stars can burn anywhere from millions to billions of years. 14 00:01:36,270 --> 00:01:43,030 \h Exactly how long they thrive for depends on the amount of gas they have to feed their nuclear furnaces. 15 00:01:43,030 --> 00:01:48,340 \h Eventually though, their fuel is exhausted and the fire goes out. 16 00:01:48,340 --> 00:01:54,520 \h Like a baby's first glimpse into the outside world, the Chandra X-ray Observatory's first sight 17 00:01:54,520 --> 00:02:01,890 \h in deep space was a bright supernova remnant called Cassiopeia A. 18 00:02:01,890 --> 00:02:04,400 \h DR. CLAUDE CANIZARES: In that very first image, we made a discovery. 19 00:02:04,400 --> 00:02:11,790 \h There was a little point source at the center, which is probably the collapsed core of the star that exploded when the 20 00:02:11,790 --> 00:02:15,430 \h supernova went off. It's either a neutron star or black hole, 21 00:02:15,430 --> 00:02:23,230 \h we're still not sure which, but people are still studying it and no one had ever seen it before. 22 00:02:23,230 --> 00:02:29,490 \h NARRATOR: Ultimately, the death of stars may spawn the formation of other new planets and stars in the universe. 23 00:02:29,490 --> 00:02:34,810 \h Such objects are made up of elements like carbon, hydrogen and iron. 24 00:02:34,810 --> 00:02:42,050 \h These elements are forged deep in the hot interior of stars and need a self-destructive explosion to unleash them. 25 00:02:42,050 --> 00:02:46,710 \h CANIZARES: What we're doing is studying essentially a star that's turned itself inside out, 26 00:02:46,710 --> 00:02:53,210 \h very conveniently, and shown us what it's made of and what atomic elements might have been generated, 27 00:02:53,210 --> 00:02:59,030 \h synthesized in the star and are being returned to the interstellar medium where they're going to eventually mix in with 28 00:02:59,030 --> 00:03:05,300 \h other material and form new stars, new planets and maybe life somewhere 29 00:03:05,300 --> 00:03:08,920 \h if there's enough of the right material and the right conditions.