1 00:00:08,780 --> 00:00:06,619 2005 yu55 is going to make a very close 2 00:00:12,049 --> 00:00:08,790 approach to the earth on the night of 3 00:00:14,270 --> 00:00:12,059 november eighth 2011 at that time its 4 00:00:16,010 --> 00:00:14,280 distance from earth will be just under 5 00:00:20,179 --> 00:00:16,020 nine tenths of the moon's distance away 6 00:00:21,590 --> 00:00:20,189 from us 2005 yu55 cannot hit earth at 7 00:00:23,029 --> 00:00:21,600 least over the interval that we can 8 00:00:24,800 --> 00:00:23,039 compute the motion reliably which 9 00:00:27,019 --> 00:00:24,810 extends for several hundred years it's 10 00:00:29,120 --> 00:00:27,029 going to be moving very rapidly as it 11 00:00:30,919 --> 00:00:29,130 traverses the sky near the earth on 12 00:00:33,620 --> 00:00:30,929 november seventh eighth ninth and tenth 13 00:00:35,060 --> 00:00:33,630 in effect it will be moving straight at 14 00:00:36,709 --> 00:00:35,070 us from one direction and then they go 15 00:00:38,930 --> 00:00:36,719 whizzing by and straight away from us in 16 00:00:40,670 --> 00:00:38,940 the other direction so it's it's motion 17 00:00:43,130 --> 00:00:40,680 across the sky will be close to 180 18 00:00:45,139 --> 00:00:43,140 degrees over the course of less than two 19 00:00:47,930 --> 00:00:45,149 days it made a close approach to earth 20 00:00:49,520 --> 00:00:47,940 about 18 months ago in April of 2010 21 00:00:51,979 --> 00:00:49,530 colleagues of ours at eros evo 22 00:00:53,720 --> 00:00:51,989 Observatory were able to observe this 23 00:00:55,910 --> 00:00:53,730 asteroid using the radar facility at 24 00:00:59,029 --> 00:00:55,920 Arecibo and they were able to obtain 25 00:01:01,400 --> 00:00:59,039 radar images that showed that this 26 00:01:03,470 --> 00:01:01,410 object is about 400 metres across on 27 00:01:06,410 --> 00:01:03,480 november eighth ninth tenth will be 28 00:01:08,179 --> 00:01:06,420 observing it again this time with both 29 00:01:10,370 --> 00:01:08,189 the air SIBO telescope and with the 30 00:01:12,109 --> 00:01:10,380 Goldstone telescope here in california 31 00:01:14,120 --> 00:01:12,119 this is the closest approach by an 32 00:01:16,039 --> 00:01:14,130 asteroid that large that we've ever 33 00:01:18,109 --> 00:01:16,049 known about in advance the radar 34 00:01:21,380 --> 00:01:18,119 telescopes that we use to observe 35 00:01:23,600 --> 00:01:21,390 asteroids are very large radio dishes if 36 00:01:25,789 --> 00:01:23,610 the Goldstone telescope is 70 meters 37 00:01:27,499 --> 00:01:25,799 which is 240 feet across so it's truly 38 00:01:29,749 --> 00:01:27,509 enormous and Arecibo is even larger 39 00:01:32,179 --> 00:01:29,759 still the Goldstone telescope has a new 40 00:01:34,010 --> 00:01:32,189 radar imaging capability which has just 41 00:01:35,600 --> 00:01:34,020 become available that will enable us to 42 00:01:37,730 --> 00:01:35,610 see much finer detail than has 43 00:01:40,039 --> 00:01:37,740 previously been possible and depending 44 00:01:41,960 --> 00:01:40,049 on how we transmit the signal we can get 45 00:01:44,330 --> 00:01:41,970 different types of data it shows us how 46 00:01:45,859 --> 00:01:44,340 big it is it can show us features on the 47 00:01:48,620 --> 00:01:45,869 asteroid it can tell us information 48 00:01:50,810 --> 00:01:48,630 about the asteroid rotation period we 49 00:01:52,039 --> 00:01:50,820 should be able to tell much better with