1 00:00:04,660 --> 00:00:07,840 [music] 2 00:00:18,119 --> 00:00:22,820 >>It's gonna be a straight FORCAST removal today, usual procedure, I think the biggest difference 3 00:00:22,820 --> 00:00:26,369 is the fact that we're right out here on the flight ramp, and we're using the cargo truck 4 00:00:26,369 --> 00:00:31,069 with the canopy on it. We'll do the un-cableing, then after that we're ready for the instrument 5 00:00:31,069 --> 00:00:37,440 removal. Then after that, they'll rotate to 17, take off the counter-weight rack, and 6 00:00:37,440 --> 00:00:44,400 take out the PI rack. The HIPO PI rack pallet is gonna go in the number three position. 7 00:00:47,299 --> 00:00:51,760 >>Today we are swapping a science instrument on the telescope. We are actually exchanging 8 00:00:51,760 --> 00:00:56,219 the FORCAST instrument with the HIPO instrument and FLITECAM instrument that mounts with it, 9 00:00:56,219 --> 00:01:02,109 in preparation for observing a Pluto occultation event in a few more days. The entire instrument 10 00:01:02,109 --> 00:01:08,140 exchange begins with disconnecting the electrical cables of the science instruments, and then 11 00:01:08,140 --> 00:01:13,280 unbolting it from the telescope flange, and then reversing that whole process. We do this 12 00:01:13,280 --> 00:01:18,000 quite often, but this is the first time we've done it in New Zealand. 13 00:01:18,000 --> 00:01:22,320 [music/background work] 14 00:02:02,400 --> 00:02:04,640 >>This is FLITECAM. 15 00:02:04,640 --> 00:02:09,590 FLITECAM is the First Light TEst Experiment CAMera for SOFIA. It's a near infrared imager 16 00:02:09,590 --> 00:02:13,810 and spectrometer that looks at light from one to five and a half microns. 17 00:02:16,080 --> 00:02:23,500 >>HIPO is an optical instrument. It's designed to observe occultations of stars by planets. 18 00:02:23,510 --> 00:02:27,900 >>FLITECAM could look at the occultation alone, but we've got a special advantage when we can co-mount 19 00:02:27,900 --> 00:02:31,660 with HIPO, because we see different wavelengths of light. 20 00:02:31,660 --> 00:02:34,840 >>When we mount them together they're called the FLIPO configuration. 21 00:02:35,760 --> 00:02:38,520 >>Every science instrument has a different weight, and the 22 00:02:38,530 --> 00:02:42,900 shape is also different, so they have a different center of mass as well. So every time we put 23 00:02:42,900 --> 00:02:48,280 on a new science instrument, we have to balance the telescope again. Every science instrument, 24 00:02:48,280 --> 00:02:52,409 again, needs a different button. Some science instruments use that button to calibrate, 25 00:02:52,409 --> 00:02:55,209 some just need it to get rid of some stray light. 26 00:02:55,209 --> 00:02:58,289 >>FLITECAM is plugged into the MCCS IRIG-B 27 00:02:58,289 --> 00:03:00,169 signal, and that's working. 28 00:03:00,169 --> 00:03:04,659 >>Thank you very much, Ted. FLITECAM, confirm you are receiving 29 00:03:04,659 --> 00:03:06,059 GPS data? 30 00:03:06,059 --> 00:03:07,359 >> Yes. 31 00:03:07,360 --> 00:03:10,059 >>I see nothing wrong over here. 32 00:03:10,059 --> 00:03:12,419 >>It takes a lot of teamwork to get everything 33 00:03:12,430 --> 00:03:17,040 ready to go, to get these instruments ready to fly, but everyone pulled together and did 34 00:03:17,040 --> 00:03:18,260 a really good job. 35 00:03:18,260 --> 00:03:23,320 >>The functional check is complete, and I'm gonna say everything is go for flight. 36 00:03:23,320 --> 00:03:27,120 >>I think everyone's excited at this point, at least I'm excited at this 37 00:03:27,129 --> 00:03:33,129 point. We've all worked really hard and prepped really well, and I think it's gonna be a great