WEBVTT FILE 1 00:00:00.020 --> 00:00:04.040 [Sound Effects] 2 00:00:04.060 --> 00:00:08.080 [Sound Effects] 3 00:00:08.100 --> 00:00:12.090 Here are a few things you might like to know about the images you see in 4 00:00:12.110 --> 00:00:16.120 Disk Detective. The red crosshairs are 2.1 5 00:00:16.140 --> 00:00:20.160 arcseconds across. The red circle is 6 00:00:20.180 --> 00:00:24.200 10.5 arcseconds in radius. The whole Disk Detective 7 00:00:24.220 --> 00:00:28.210 image is 60 arcseconds across. An 8 00:00:28.230 --> 00:00:32.260 arcsecond is about the size of a dime seen from a mile away. 9 00:00:32.280 --> 00:00:36.280 For example: the angular diameter of the planet Neptune as 10 00:00:36.300 --> 00:00:40.300 seen from Earth is about 150 arcseconds. 11 00:00:40.320 --> 00:00:44.330 In these images, the bright objects appear white 12 00:00:44.350 --> 00:00:48.380 or light blue. The empty sky around them 13 00:00:48.400 --> 00:00:52.420 appears black or a mottled black-and-blue pattern. 14 00:00:52.440 --> 00:00:56.440 That mottling is noise. You'll want to focus your 15 00:00:56.460 --> 00:01:00.470 attention on the white and light-blue areas. At 16 00:01:00.490 --> 00:01:04.490 Disk Detective, we find new disks by looking at the object 17 00:01:04.510 --> 00:01:08.540 in images taken with several different telescopes. The images are 18 00:01:08.560 --> 00:01:12.610 arranged in a flip book, which you can play by clicking on the play button on the lower left. 19 00:01:12.630 --> 00:01:16.620 A good candidate is small and round 20 00:01:16.640 --> 00:01:20.640 and mostly contained within the red circle--like this object. 21 00:01:20.660 --> 00:01:24.690 Sometimes bright objects, like this one on the left, 22 00:01:24.710 --> 00:01:28.710 can have diffraction spikes that stick out beyond the red circle. These can 23 00:01:28.730 --> 00:01:32.720 also be good candidates. We're not as interested in objects that are 24 00:01:32.740 --> 00:01:36.740 outside the red circle, but if you like you can click on 25 00:01:36.760 --> 00:01:40.750 the icon in the upper right and discuss them on talk. 26 00:01:40.770 --> 00:01:44.810 Here on the talk page, you can see the image ID 27 00:01:44.830 --> 00:01:48.830 in the upper-left-hand corner. You can also click on the 28 00:01:48.850 --> 00:01:52.880 collect button to favorite your image, to start a collection of your 29 00:01:52.900 --> 00:01:56.900 favorite images. You can type your own comments 30 00:01:56.920 --> 00:02:00.960 into the blue box, and you can read comments that 31 00:02:00.980 --> 00:02:04.980 other people have written. SED stands 32 00:02:05.000 --> 00:02:09.040 for Spectral Energy Distribution. That's a plot 33 00:02:09.060 --> 00:02:13.060 of how bright this object is in each of the infrared wavelengths 34 00:02:13.080 --> 00:02:17.100 that you saw in the flip book. Looking at SEDs 35 00:02:17.120 --> 00:02:21.140 can help us figure out whether the object is really a star with a disk 36 00:02:21.160 --> 00:02:25.160 or whether it's some other kind object, maybe a galaxy. 37 00:02:25.180 --> 00:02:29.220 Click on the "More info in SIMBAD" button to access a powerful 38 00:02:29.240 --> 00:02:33.250 database of astronomical objects. This 39 00:02:33.270 --> 00:02:37.280 line in SIMBAD tells you the angular distance in arcseconds 40 00:02:37.300 --> 00:02:41.330 between the Disk Detective object and this SIMBAD object 41 00:02:41.350 --> 00:02:45.350 to help you make sure you are looking at the right thing. SIMBAD is a great 42 00:02:45.370 --> 00:02:49.380 resource, but doesn't have information on every Disk Detective 43 00:02:49.400 --> 00:02:53.410 object. Also, SIMBAD is sometimes wrong, so don't 44 00:02:53.430 --> 00:02:57.440 discount an object just because SIMBAD has labeled it as a quasar, 45 00:02:57.460 --> 00:03:01.470 like this one. If you use a 46 00:03:01.490 --> 00:03:05.530 hashtag in your comments, people will be able to find your comments easily 47 00:03:05.550 --> 00:03:09.570 by searching for that hashtag. After you've watched the flip book 48 00:03:09.590 --> 00:03:13.600 at least once, you can select the classification of this object 49 00:03:13.620 --> 00:03:17.630 by clicking on the rectangles. This looks like a good candidate 50 00:03:17.650 --> 00:03:21.660 since it looks round, and fairly concentrated, so I'll click "None 51 00:03:21.680 --> 00:03:25.700 of the Above/Good Candidate" Then I'll click on the 52 00:03:25.720 --> 00:03:29.730 "Finish" button to record my classification. 53 00:03:29.750 --> 00:03:33.780 If you've gotten this far, congratulations, you've just classified 54 00:03:33.800 --> 00:03:37.810 an object. Thank you for helping NASA find new planetary 55 00:03:37.830 --> 00:03:41.850 systems. 56 00:03:41.870 --> 00:03:45.900 57 00:03:45.920 --> 00:03:49.930 [Beeping] 58 00:03:49.950 --> 00:03:58.352 [Beeping]