7 Eye-Opening Facts About Venus

For all the efforts to find another inhabitable planet orbiting a distant star, it might surprise you to learn that a very real Earth 2.0 exists in this solar system—just one planet over. Not Mars (which actually isn't much like Earth at all), but rather, our other neighbor: Venus. Mental Floss spoke to geophysicist Bob Grimm, a program director at the Southwest Research Institute and chair of NASA's Venus Exploration Analysis Group. Here are a few things we learned about Earth's twin sister.


Venus has a radius of 3760 miles. Earth's is 3963. Its mass and gravity are 82 percent and 91 percent of Earth's, respectively—pretty similar as planets go. Venus is composed of a mostly basalt crust, silicate mantle, and iron core. Earth is the same. The two planets likely share common origins somewhere around 4.5 billion years ago.

In fact, by all accounts, we should be able to land our flying saucers on Venus, saddle up a dinosaur, and start building tract housing. It's perfect for colonization, but for a few minor differences. Its year is shorter, at 224.7 days. (And its days are much longer, at 243 Earth days per Venus day.) The Sun would rise in the west and set in the east because of the planet's retrograde orbit (which, by the way, is the most circular of any planet in the solar system). And then there's another small problem …


Venus is hotter than Mercury, despite being 30 million miles farther from the Sun. How hot? Hot enough, on average, to melt a block of lead the way a block of ice would melt on Earth. Venus suffers from a runaway greenhouse effect. Sunlight penetrates the dense clouds surrounding Venus, heating the landscape. The ground in turn blasts out heat, which rises and tries to escape the atmosphere. But carbon dioxide, which makes up 96 percent of its atmosphere, traps the heat, keeping things nice and toasty, around 900°F. And those clouds aren't the white, fluffy variety. They're made of droplets of sulfuric acid, which makes its lightning storms especially harrowing.


"'Does Earth-size mean Earth-like?' is a basic problem of planetology," says Grimm. "Understanding how Earth and Venus diverged is essential to understanding comparative planetology, and potentially exoplanets—these worlds orbiting distant stars that are being discovered telescopically."

Knowing more about Venus would help scientists better distinguish potentially habitable worlds out there, and better understand how a good world can go bad, from a sustaining-life perspective. "Geology and meteorology are intimately related to the evolution of the Earth and the evolution of life on Earth," Grimm notes. "Even though we may not be looking for life on Venus, it's important to understanding Earth's place in the solar system and in the universe."


You might have run across old illustrations of Venus with conditions similar to the Carboniferous Period on Earth. Astronomers have known for just under a hundred years that Venus's atmosphere is devoid of oxygen, without which you can't have water. But even a modest backyard telescope can see the clouds enveloping our neighbor, and as Carl Sagan explained, from there you're only a couple of erroneous jumps from assuming a brontosaurus. (Thick clouds mean more water than land. More water than land means swamps. Dinosaurs lived in swamps. Dinosaurs live on Venus. QED.) Said Sagan: "Observation: There was absolutely nothing to see on Venus. Conclusion: It must be covered with life."

But seeing is believing, and the Mariner and Venera series of probes disabused us of the romantic notion of a swampy neighbor to the left. Still, we should probably send robots there to check. Just to be sure.


Venus was the first planet we visited, with Mariner 2 achieving the first successful planetary encounter in 1962. Four years later, Venera 3 on Venus became the first spacecraft to touch the surface of another planet. (Communications were lost long before impact, but unless a dinosaur ate it, the spacecraft probably touched the ground.) Our first graceful landing on another planet? Venera 7 on Venus. Our efforts to reach its surface go back much further than that, though. The transit of Venus in 1761 practically invented the notion of an international science community. But we abandoned the surface of Venus in 1984, and NASA hasn't launched an orbiter to Venus since Magellan in 1989. 

Since then, the Venus-science community has been trying to get another mission to the launch pad. Presently, U.S. planetary scientists have submitted proposals to NASA for a sub-$1 billion New Frontiers–class mission. They are also working with their colleagues in Russia to launch a joint mission called Venera-D. "We need better radar views of the surface," says Grimm, "and that has to happen at some point to understand the geology. We need deep probes into the atmosphere to understand it better, and we need a new generation of landers."


"There is evidence in the deuterium-to-hydrogen ratio that Venus once had water, maybe hundreds of meters deep, more like a global sea than an ocean," says Grimm. A theoretical paper published last year posed a climate model for Venus suggesting that water could have existed on its surface as recently as 1 billion years ago. Clouds could form in a certain way, shielding the surface from the Sun and allowing stable water at the surface. Furthermore, near-infrared observations support the argument for a watery Venusian past. ESA's Venus Express orbiter in 2012 found evidence of granite-like rocks on some parts of the planet. Granite requires a multiple melting process in the presence of water. A mission to Venus could confirm this.

Meanwhile, one of the most significant revelations from Magellan is that there are only around 1000 craters on the surface with no differences in density, and it is hard to find craters that are obviously in a state of being wiped out by lava, or being faulted. Venus does not have plate tectonics, one of the central mechanisms that organizes all geology on the Earth. So what happened to the surface of Venus? Where is the evidence of the Late Heavy Bombardment seen on other terrestrial planets and moons? One hypothesis is that all of Venus was resurfaced at once. There may have been a global catastrophe on Venus, perhaps as recently 750 million years ago, that quickly "reset" its surface. Other models suggest a subtler resurfacing at work in which craters might be erased over billions of years.

"So this whole idea of the surface age of Venus is a pivotal question for how planets evolve geologically," says Grimm. "But what was Venus like before that? Was there a single catastrophe, or have there been many? Was there just one catastrophe and Venus was watery before that, or has Venus operated in a steady state going back to the first billion years? There is more consensus that in the first several hundred million years to billion years, there could have been water." Further landings on Venus could help us solve the mystery of when Venus's surface was formed, if there was ever water there, and why, if it existed, it went away.


If Matt Damon were to get stranded on Venus in a sequel to The Martian, he would need to be resourceful indeed to survive the heat and the corrosive air. But what he would find wouldn't be wholly alien. The winds at the surface of Venus are very gentle, around a meter or so per second. The vistas would consist of hills and ridges, with dark lava rocks of various types, mostly basalt. The atmospheric pressure is 90 times greater than Earth at sea level, so walking there would feel a lot like swimming here.

"I don't think [Venus] would look wavy and hot-hazy, because the atmosphere is pretty stable and uniform right at the surface," says Grimm. "It would be harder to walk through the dense atmosphere, but not as hard as walking through water. We know from landings that it's kind of yellow because of the sulfur in the atmosphere. So with the abundance of lavas in many places on Venus, it sort of looks like a yellowish Hawaii."

A Snow Moon—the Year’s Brightest Supermoon—Will Be Visible Next Week


Save the date: The next supermoon is set to light up skies on Tuesday, February 19. Because of when it's arriving, the event will also be a snow moon—a type of full moon that can only been seen this time of year, USA Today reports.

What is a supermoon?

A supermoon occurs when the moon is at its largest in the night sky. That means the Moon is not only full, but also at the point in its orbit that brings it closest to Earth—a position called perigee. On Tuesday, the Moon will appear 14 percent larger and 30 percent brighter than when it's farthest from our planet, making it the brightest supermoon of 2019.

This next supermoon will also have a fun nickname that fits the season. The full moon of each month has a special name. A harvest moon, the first full moon of September, is the best-known moniker, but there are also strawberry moons (June), sturgeon moons (August), and so on. A snow moon is the name for the full moon in February, alluding to February being the snowiest month of the year in the U.S.

When to watch the next supermoon

If the weather is clear in your area, the best time to see the super snow moon is early Tuesday morning on February 19, when the moon reaches its perigee. The Moon will become officially full six hours later at 10:53 a.m. EST. Sunday, Monday, and Tuesday nights will also offer spectacular views of a seemingly huge, nearly full moon.

Supermoons usually happen just a few times a year, but skygazers won't have to wait long for the next one: There's a super worm moon coming March 21, 2019.

[h/t USA Today]

11 Photos From the Opportunity Rover's Mission on Mars


In 2004, the rover Opportunity landed on Mars. Originally intended to serve a mere 90-day mission, the rover instead beamed back scientific discoveries for 15 years. But since a massive dust storm in 2018, the rover Opportunity ceased sending data—and now, NASA has declared its groundbreaking mission complete. (Its twin rover, Spirit, ended its mission in 2011.) Opportunity is the longest-serving robot ever sent to another planet. Let's celebrate Opportunity's Mars mission with a look at the images it captured.

1. Opportunity rover gets its first 360° shot.

Rover Opportunity's 360° photo of Mars

This 360° panorama, comprised of 225 frames, shows Mars as it was seen by the Opportunity rover on February 2, 2004. You can see marks made by the rover's airbags, made as Opportunity rolled to a stop. Here's a larger version of the photo.

2. Opportunity rover finds a meteorite.

Opportunity rover's photo of a meteorite on Mars

This meteorite, found by Opportunity on January 19, 2005, was the first meteorite ever identified on another planet. The rover's spectrometers revealed that the basketball-sized meteorite was composed mostly of iron and nickel.

3. Opportunity rover shoots the Erebus Crater and drifts.

Opportunity rover's photo of Erebus craters and drift

On October 5, 2005—four months after Opportunity got stuck in an area NASA nicknamed "Purgatory Dune"—the rover skirted wind-deposited drifts in the center of the Erebus Crater, heading west along the outcrop (the light-toned rock) on the crater's rim, and snapped this photo with its PanCam.

4. Opportunity rover captures Martian rock layers.

Opportunity rover's photo of layers on Mars

Located on the western ledge of the Erebus Crater, this ledge—called "Payson"—has a diverse range of primary and secondary sedimentary layers formed billions of years ago. According to NASA, "these structures likely result from an interplay between windblown and water-involved processes." Opportunity snapped this photo on April 5, 2006.

5. Opportunity rover comes to Cape Verde.

Opportunity rover's photo of Cape Verde

On October 20, 2007, Opportunity celebrated its second Martian birthday (one Martian year = 687 Earth days) by snapping this photo of Cape Verde, a promontory that juts out of the wall of the Victoria Crater. Scattered light from dust on the front sapphire window of the rover's camera created the soft quality of the image and the haze in the right corner.

6. and 7. Opportunity rover is hard at work on Marquette Island.

Opportunity rover's photo of Marquette Island

This photo shows Opportunity approaching a rock called "Marquette Island" on November 5, 2009. Because its dark color made it stick out, the rover team referred to the rock—which investigations suggested was a stony meterorite—as "Sore Thumb." But it was eventually renamed, according to NASA, using "an informal naming convention of choosing island names for the isolated rocks that the rover is finding as it crosses a relatively barren plain on its long trek from Victoria Crater toward Endeavour Crater."

On November 19, 2009, the rover used its rock abrasion tool to analyze a 2-inch diameter area of Marquette, which scientists called "Peck Bay."

8. Opportunity rover encounters SkyLab Crater.

Opportunity rover's photo of SkyLab Crater

Opportunity snapped a photo of this small crater, informally called Skylab, on May 12, 2011. Scientists estimate that the 30-foot crater was formed within the past 100,000 years. Click the photo for a larger version. You can also see the crater in stereo if you have a pair of anaglyph glasses!

9. Opportunity rover sees its shadow.

Opportunity rover's selfie

On its 3051st day on Mars (August 23, 2012), Opportunity snapped this photo of its own shadow stretching into the Endeavour Crater.

10. Opportunity rover sees its first dust devil.

Opportunity rover's photo of a dust devil
NASA/JPL-Caltech/Cornell University/Texas A&M

Though its twin rover, Spirit, had seen many dust devils by this point, Opportunity caught sight of one for the first time on July 15, 2010.

11. Opportunity rover snaps a selfie.

Opportunity rover's self-portrait
NASA/JPL-Caltech/Cornell University/Arizona State University

A girl sure can get dusty traversing the Martian plains! Opportunity snapped the images that comprise this self-portrait with its panoramic camera between January 3 and January 6, 2014, a few days after winds blew off some of the dust on its solar panels. The shadow belongs to the mast—which is not in the photo—that the PanCam is mounted on.