1 00:00:00,390 --> 00:00:03,259 Hubble makes an exoplanet discovery … 2 00:00:03,259 --> 00:00:05,870 The next space station crew gets ready to launch … 3 00:00:05,870 --> 00:00:11,430 And back to work in Florida after weathering the storm … a few of the stories to tell 4 00:00:11,430 --> 00:00:14,880 you about – This Week at NASA! 5 00:00:14,880 --> 00:00:19,300 Researchers using data from our Hubble Space Telescope have, for the first time, detected 6 00:00:19,300 --> 00:00:25,179 water vapor signatures in the atmosphere of a planet outside our solar system that resides 7 00:00:25,179 --> 00:00:26,800 in the "habitable zone." 8 00:00:26,800 --> 00:00:31,199 This is the region around a star in which liquid water could potentially pool on the 9 00:00:31,199 --> 00:00:33,440 surface of a rocky planet. 10 00:00:33,440 --> 00:00:39,800 The planet – known as K2-18b, orbits a small red dwarf star about 110 light-years from 11 00:00:39,800 --> 00:00:42,030 us, in the constellation Leo. 12 00:00:42,030 --> 00:00:47,329 If confirmed by further studies, this will be the only exoplanet known to have both water 13 00:00:47,329 --> 00:00:54,539 in its atmosphere and temperatures that could sustain liquid water on a rocky surface. 14 00:00:54,539 --> 00:00:58,680 The next crew headed to the International Space Station, including our Jessica Meir, 15 00:00:58,680 --> 00:01:04,070 wrapped up activities at the Gagarin Cosmonaut Training Center outside Moscow on Sept. 10. 16 00:01:04,070 --> 00:01:09,450 Meir and her crewmates – Oleg Skripochka of Roscosmos, and Spaceflight Participant 17 00:01:09,450 --> 00:01:15,490 Hazzaa Ali Almansoori – then departed for the Baikonur Cosmodrome launch site in Kazakhstan 18 00:01:15,490 --> 00:01:17,530 to complete their training. 19 00:01:17,530 --> 00:01:23,080 The trio is scheduled to launch to the station on Sept. 25. 20 00:01:23,080 --> 00:01:28,170 On Sept. 10 at our Kennedy Space Center in Florida, the mobile launcher for our Artemis 21 00:01:28,170 --> 00:01:34,230 missions to the Moon began the 4-mile ride atop crawler-transporter 2 back to Launch 22 00:01:34,230 --> 00:01:39,979 Pad 39B – after being housed for more than a week inside the Vehicle Assembly Building 23 00:01:39,979 --> 00:01:42,100 due to Hurricane Dorian. 24 00:01:42,100 --> 00:01:47,180 With the mobile launcher back in place at the pad, teams can resume validation and verification 25 00:01:47,180 --> 00:01:52,540 testing for our Artemis I mission – which they plan to complete in the coming weeks. 26 00:01:52,540 --> 00:01:57,940 Artemis I will be the first integrated uncrewed test flight of our Orion spacecraft, Space 27 00:01:57,940 --> 00:02:03,590 Launch System or SLS rocket and the ground systems at Kennedy Space Center. 28 00:02:03,590 --> 00:02:08,840 Meanwhile, progress toward the launch pad for Artemis I continues for our SLS rocket 29 00:02:08,840 --> 00:02:10,570 and Orion spacecraft. 30 00:02:10,570 --> 00:02:16,690 SLS and Orion have moved from design and manufacturing, to testing and assembly and integration – some 31 00:02:16,690 --> 00:02:20,340 of the hardware has even been delivered to the launch pad at Kennedy. 32 00:02:20,340 --> 00:02:25,840 A new online animated video shows a breakdown of the parts that will make up the completed 33 00:02:25,840 --> 00:02:27,650 flight hardware for the mission. 34 00:02:27,650 --> 00:02:31,819 Check it out at go.nasa.gov/artemis1progress. 35 00:02:31,819 --> 00:02:37,319 Along with the Gateway in lunar orbit and a new human landing system, SLS and Orion 36 00:02:37,319 --> 00:02:45,130 create the backbone for our Artemis missions that will land astronauts on the Moon by 2024. 37 00:02:45,130 --> 00:02:50,629 Radar data from our Cassini spacecraft were used in recently published research that suggests 38 00:02:50,629 --> 00:02:56,600 explosions of warming liquid nitrogen are responsible for the steep-rimmed craters encircling 39 00:02:56,600 --> 00:03:00,879 some of the methane-filled lakes on Saturn’s moon Titan. 40 00:03:00,879 --> 00:03:05,860 Most existing models that lay out the origin of Titan's lakes point to a process that does 41 00:03:05,860 --> 00:03:08,349 not produce steep rims. 42 00:03:08,349 --> 00:03:13,540 Titan and Earth are the only planetary bodies in our solar system known to have stable surface 43 00:03:13,540 --> 00:03:19,230 liquids – water on Earth and methane and ethane on Titan — hydrocarbons that we think 44 00:03:19,230 --> 00:03:24,200 of as gases, but that behave as liquids in Titan's frigid climate. 45 00:03:24,200 --> 00:03:29,720 The radar data were gathered during Cassini’s last close flyby of Titan, as the spacecraft 46 00:03:29,720 --> 00:03:34,209 prepared for its final plunge into Saturn's atmosphere two years ago. 47 00:03:34,209 --> 00:03:37,989 That’s what’s up this week @NASA …