On flyby, NASA’s solar mission observed the hot glow from the nightside surface, capturing the first optical images of the hidden ground under the clouds since the 1982 visits of the Venera 13 and 14 landers
9 February 2022
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WASHINGTON — On a flyby of Venus, NASA’s Parker Solar Probe captured the first visible light images of the cloudy planet’s surface from space, a new study reports. The nightside view of the extremely hot surface could help scientists understand the contrasting evolution of Earth’s nearest neighbor.
Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entirety of the nightside in wavelengths of the visible spectrum – the type of light that the human eye can see — and extending into the near-infrared.
The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet, according to the new study in AGU’s journal Geophysical Research Letters, which publishes high-impact, short-format reports with immediate implications spanning all Earth and space sciences.
Such images of the planet, often called Earth’s twin, can help scientists learn more about Venus’ surface geology, what minerals might be present there, and the planet’s evolution. Given the similarities between the planets, this information can help scientists on the quest to understand why Venus became inhospitable and Earth became an oasis.
“Venus is the third brightest thing in the sky, but until recently we have not had much information on what the surface looked like because our view of it is blocked by a thick atmosphere,” said Brian Wood, lead author on the new study and physicist at the Naval Research Laboratory in Washington, DC. “Now, we finally are seeing the surface in visible wavelengths for the first time from space.”
Glowing like an iron from the forge
Clouds obstruct most of the visible light coming from Venus’ surface, but the very longest visible wavelengths, which border the near-infrared wavelengths, make it through. On the dayside, this red light gets lost amid the bright sunshine reflected off Venus’ cloud tops, but in the darkness of night, the WISPR camera was able to pick up this faint glow caused by the incredible heat emanating from the surface.
As Parker Solar Probe flew by Venus on its fourth flyby, its WISPR instrument captured these images, strung into a video, showing the nightside surface of the planet.
Credits: NASA/APL/NRL
“The surface of Venus, even on the nightside, is about 860 degrees [Fahrenheit],” Wood said. “It’s so hot that the rocky surface of Venus is visibly glowing, like a piece of iron pulled from a forge.”
As it passed by Venus, WISPR picked up a range of wavelengths from 470 nanometers to 800 nanometers. Some of that light is the near-infrared – wavelengths that we cannot see, but sense as heat – and some is in the visible range, between 380 nanometers and about 750 nanometers.
Venus in a new light
In 1975, the Venera 9 lander sent the first tantalizing glimpses of the surface after landing on Venus. Since then, Venus’ surface has been revealed further with radar and infrared instruments, which can peer through the thick clouds by using wavelengths of light invisible to the human eye. NASA’s Magellan mission created the first maps in the 1990s using radar and JAXA’s Akatsuki spacecraft gathered infrared images after reaching orbit around Venus in 2016. The new images from Parker add to these findings by extending the observations to red wavelengths at the edge of what we can see.
The WISPR images show features on the Venusian surface, such as the continental region Aphrodite Terra, the Tellus Regio plateau, and the Aino Planitia plains. Since higher altitude regions are about 85 degrees Fahrenheit cooler than lower areas, they show up as dark patches amidst the brighter lowlands. These features can also be seen in previous radar images, such as those taken by Magellan.
Beyond looking at surface features, the new WISPR images will help scientists better understand the geology and mineral make-up of Venus. When heated, materials glow at unique wavelengths. By combining the new images with previous ones, scientists now have a wider range of wavelengths to study, which can help identify what minerals are on the surface of the planet. Such techniques have previously been used to study the surface of the Moon. Future missions will continue to expand this range of wavelengths, which will contribute to our understanding of habitable planets.
This information could also help scientists understand the planet’s evolution. While Venus, Earth, and Mars all formed around the same time, they are very different today. The atmosphere on Mars is a fraction of Earth’s while Venus has a much thicker atmosphere. Scientists suspect volcanism played a role in creating the dense Venusian atmosphere, but more data are needed to know how. The new WISPR images might provide clues about how volcanos may have affected the planet’s atmosphere.
In addition to the surface glow, the new images show a bright ring around the edge of the planet caused by oxygen atoms emitting light in the atmosphere. Called airglow, this type of light is also present in Earth’s atmosphere, where it’s visible from space and sometimes from the ground at night.
Unexpected Capabilities
While Parker Solar Probe’s primary goal is solar science, the Venusian flybys are providing exciting opportunities for bonus data that wasn’t expected at the mission’s launch.
“We’re thrilled with the science insights Parker Solar Probe has provided thus far,” said Nicola Fox, division director for the Heliophysics Division at NASA Headquarters. “Parker continues to outperform our expectations, and we are excited that these novel observations taken during our gravity assist maneuver can help advance Venus research in unexpected ways.”
The first WISPR images of Venus were taken in July 2020 as Parker embarked on its third flyby, which the spacecraft uses to bend its orbit closer to the Sun. WISPR was designed to see faint features in the solar atmosphere and wind, and some scientists thought they might be able to use WISPR to image the cloud tops veiling Venus as Parker passed the planet.
A dense layer of toxic clouds swath Venus, seen by NASA’s Mariner 10 spacecraft in February 1974. The clouds whip around the planet at about 100 meters per second (200 miles per hour), circling the globe in about four and a half days.
Credit: NASA/JPL-Caltech
“The objective was to measure the speed of the clouds,” said WISPR project scientist Angelos Vourlidas, co-author on the new paper and researcher at Johns Hopkins University Applied Physics Laboratory.
But instead of just seeing clouds, WISPR also saw through to the surface of the planet. The images were so striking that the scientists turned on the cameras again during the fourth pass in February 2021. During the 2021 flyby, the spacecraft’s orbit lined up perfectly for WISPR to image Venus’ nightside in entirety.
“The images and video just blew me away,” Wood said.
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Notes for Journalists:
This research study is open access. Download a PDF copy of the paper here. Neither the paper nor this press release is under embargo.
Paper title:
“Parker Solar Probe Imaging of the Night Side of Venus”
Authors:
- Brian Wood, corresponding author (Naval Research Laboratory)
- Phillip Hess (Naval Research Laboratory)
- Jacob Lustig-Yaeger (The Johns Hopkins University Applied Physics Laboratory)
- Brendan Gallagher (Naval Research Laboratory)
- Daniel Korwan (Naval Research Laboratory)
- Nathan Rich (Naval Research Laboratory)
- Guillermo Stenborg (The Johns Hopkins University Applied Physics Laboratory)
- Arnaud Thernisien (Naval Research Laboratory)
- Syed Qadri (Naval Research Laboratory)
- Freddie Santiago (Naval Research Laboratory)
- Javier Peralta (Universidad de Sevilla)
- Giada Arney (NASA Goddard Space Flight Center)
- Noam Izenberg (The Johns Hopkins Applied Physics Laboratory)
- Angelos Vourlidas (The Johns Hopkins University Applied Physics Laboratory)
- Mark Linton (Naval Research Laboratory)
- Russell Howard (The Johns Hopkins University Applied Physics Laboratory)
- Nour E. Raouafi (The Johns Hopkins University Applied Physics Laboratory)