WEBVTT FILE 1 00:00:00.530 --> 00:00:06.720 NASA has captured the first visible light images of the surface of Venus from space. 2 00:00:06.720 --> 00:00:13.400 The planet’s surface is normally shrouded from sight by a thick layer of clouds. 3 00:00:13.400 --> 00:00:20.620 But in 2020 and 2021, Parker Solar Probe pointed its cameras at the nightside of Venus as the spacecraft flew by. 4 00:00:20.620 --> 00:00:26.850 The cameras are known as the Wide-Field Imager for Solar Probe, or WISPR. 5 00:00:26.850 --> 00:00:33.560 WISPR was designed to see faint features in the solar wind flowing out from the Sun. 6 00:00:33.560 --> 00:00:39.830 Scientists thought they could use the cameras to see Venus’ clouds during flybys of the planet. 7 00:00:39.830 --> 00:00:45.060 Instead, they saw light and dark surface features through the clouds. 8 00:00:45.060 --> 00:00:50.220 This is the first time visible light from the Venusian surface has been captured from space. 9 00:00:50.220 --> 00:00:53.620 It's thrilling to be able to see something that's never been seen before. 10 00:00:53.620 --> 00:00:56.250 This emission that we're seeing is thermal emission. 11 00:00:56.250 --> 00:00:59.310 Even on the nightside, the surface of Venus is so hot 12 00:00:59.310 --> 00:01:05.690 that it's glowing faintly at very red wavelengths. 13 00:01:05.690 --> 00:01:12.280 In the images, light areas are hotter and dark areas are cooler. 14 00:01:12.280 --> 00:01:19.270 These WISPR images are really exciting because they provide a new window into the lower atmosphere 15 00:01:19.270 --> 00:01:24.910 and surface region of Venus where these extreme conditions exist. 16 00:01:24.910 --> 00:01:33.600 Scientists compared the WISPR images to topographical maps created with radar to see how temperatures change with altitude. 17 00:01:33.600 --> 00:01:39.930 This is Aphrodite Terra, the largest highland region on Venus. 18 00:01:39.930 --> 00:01:47.710 Higher elevations tend to be cooler, and lowland regions hotter. 19 00:01:47.710 --> 00:01:53.630 The images could also help scientists see other heat variations. 20 00:01:53.630 --> 00:01:59.620 Another really interesting thing we can look for is potentially mineralogical differences. 21 00:01:59.620 --> 00:02:04.400 Different rocks, different minerals emit different levels of heat. 22 00:02:04.400 --> 00:02:10.110 Understanding the composition of the surface could teach about the planet’s evolution. 23 00:02:10.110 --> 00:02:17.420 Today, Venus is inhospitable to life with extreme temperatures, toxic clouds, and a crushing atmosphere. 24 00:02:17.420 --> 00:02:22.680 But the planet may have had a different past. 25 00:02:22.680 --> 00:02:27.580 We have chemical fingerprints in Venus’ atmosphere and on its surface 26 00:02:27.580 --> 00:02:31.730 suggesting that Venus may have been habitable in the past. 27 00:02:31.730 --> 00:02:41.930 The only other visible light images of the surface of Venus were taken by the Soviet Union’s Venera program when spacecraft landed on the planet. 28 00:02:41.930 --> 00:02:50.990 Since then, we have studied Venus with infrared and radar instruments that can peer through the dense atmosphere. 29 00:02:50.990 --> 00:02:57.910 The WISPR images extend our observations to red visible light at the edge of what the human eye can see. 30 00:02:57.910 --> 00:03:04.170 Parker Solar Probe will have a final chance to image Venus in 2024 31 00:03:04.170 --> 00:03:10.460 and scientists hope the WISPR images will collectively have a lasting impact on Venus research. 32 00:03:10.460 --> 00:03:18.580 This is something that's truly new, and I believe will yield exciting, exciting science in the long term. 33 00:03:18.580 --> 00:03:24.907