WEBVTT FILE 1 0:00:00.000 --> 0:00:07.520 OSIRIS-REx's Two Spectrometers 2 0:00:07.680 --> 0:00:11.060 OSIRIS- REx has two spectrometers onboard. One is the visible and near 3 0:00:11.060 --> 0:00:15.360 infrared spectrometer OVIRS and the other is the farther infrared 4 0:00:15.360 --> 0:00:17.280 spectrometer OTES. 5 0:00:17.340 --> 0:00:19.700 OVIRS is specifically looking at the reflected 6 0:00:19.710 --> 0:00:23.460 sunlight in the visible wavelength region. So basically, we can see which 7 0:00:23.460 --> 0:00:27.599 minerals are absorbing the sunlight and it extends a little bit into the thermal 8 0:00:27.599 --> 0:00:31.120 Infrared, which is the heat signature coming off the surface. 9 0:00:31.120 --> 0:00:32.130 OTES 10 0:00:32.130 --> 0:00:35.610 is farther in the infrared, well beyond where your eye can see and it's more 11 0:00:35.610 --> 0:00:39.239 sensitive to the thermal signature of the surface. Using that you can look for 12 0:00:39.239 --> 0:00:42.899 minerals, but you can also look to see how the different grains on the surface 13 0:00:42.899 --> 0:00:46.140 hold heat and then later release them and this tells us a lot about the 14 0:00:46.140 --> 0:00:50.430 surface structure as well as the composition. So combined these two 15 0:00:50.430 --> 0:00:54.930 spectrometers are an incredibly powerful suite of being able to sense the 16 0:00:54.930 --> 0:00:58.780 temperatures and composition at the same time on the surface.