1 00:00:00,000 --> 00:00:03,180 Narrator: The most comprehensive dataset from NASA's 2 00:00:03,180 --> 00:00:05,650 Kepler Mission will help researchers discover 3 00:00:05,650 --> 00:00:09,440 how many Earth-size\hplanets are in our galaxy.\h 4 00:00:09,440 --> 00:00:12,070 Using\hthe first\hfour years of Kepler observations 5 00:00:12,070 --> 00:00:14,140 in the constellation of Cygnus, 6 00:00:14,140 --> 00:00:16,090 the\hPlanet Candidate Catalog\hcontains 7 00:00:16,090 --> 00:00:19,150 the best characterized data yet. 8 00:00:19,150 --> 00:00:23,520 The data contains 219 new planet candidates. 9 00:00:23,520 --> 00:00:26,130 Ten of these are less than twice the size of 10 00:00:26,130 --> 00:00:30,250 the Earth and orbit in their stars' habitable zones. 11 00:00:30,250 --> 00:00:32,960 The habitable zone is a range of distance from a 12 00:00:32,960 --> 00:00:35,660 star where liquid water could pool on the surface 13 00:00:35,660 --> 00:00:37,860 of a rocky planet. 14 00:00:37,860 --> 00:00:40,100 The data will be used by scientists to help 15 00:00:40,100 --> 00:00:42,690 determine the frequency and variety of planets 16 00:00:42,690 --> 00:00:44,760 in the galaxy. 17 00:00:44,760 --> 00:00:47,910 A recent discovery using Kepler data showed that 18 00:00:47,910 --> 00:00:51,850 small planets come in two distinct size classes: 19 00:00:51,850 --> 00:00:54,700 The Earth and super-Earth-size class and 20 00:00:54,700 --> 00:00:59,010 the slightly larger mini-Neptune-size class. 21 00:00:59,010 --> 00:01:02,680 The result shows that nature commonly makes rocky 22 00:01:02,680 --> 00:01:06,690 planets up to about 75 percent bigger than Earth. 23 00:01:06,690 --> 00:01:09,630 Kepler has identified more than 4,000 planet 24 00:01:09,630 --> 00:01:12,090 candidates beyond the solar system and 25 00:01:12,090 --> 00:01:17,640 2,335 of which have been confirmed as planets. 26 00:01:17,640 --> 00:01:20,780 Kepler's search for planets continues as part of 27 00:01:20,780 --> 00:01:24,600 an on-going study of different regions of space.