Two Exoplanets May Be Mostly Water, NASA's Hubble and Spitzer Find

December 15, 2022 11:00AM (EST)Release ID: 2022-048
Illustration of three planets and their star on the black background of space speckled with dots of different colors. The planets are various sizes, indicating different distances from the viewer and from the star. The star is near the middle of the illustration. The smallest planet in the illustration, which is closest to the star and farthest from the viewer, appears as a small black dot on the star. The largest, foreground planet, is at the upper right. The planet is grayish white with bands of clouds. The left one-eighth or so of the planet (the portion facing the star) is lit; the rest is in shadow. A third planet, middle-sized on the illustration, lies to the left of the star, in between the two other planets in terms of apparent distance from the star and from the viewer. There are no discernible features on the planet. The right one-eighth (the portion facing the star) is lit; the rest is in shadow. The star is bright orange-yellow, with no clear features.

Summary

Pair of Super-Earths Have 1,000-Mile-Deep Oceans

In the 1995 post-apocalyptic action film "Waterworld" Earth's polar ice caps have completely melted, and the sea level has risen to over 5 miles, covering nearly all of the land. Astronomers have uncovered a pair of planets that are true "water worlds," unlike any planet found in our solar system.

Slightly larger than Earth, they don't have the density of rock. And yet, they are denser than the gas-giant outer planets orbiting our Sun. So, what are they made of? The best answer is that these exoplanets have global oceans at least 500 times deeper than the average depth of Earth's oceans, which simply are a wet veneer on a rocky ball.

The soggy worlds orbit the red dwarf star Kepler-138, located 218 light-years away in the constellation Lyra. The planets were found in 2014 with NASA's Kepler Space Observatory. Follow-up observations with the Spitzer and Hubble space telescopes found that the planets must be composed largely of water. The spectral signature of water wasn't directly observed. But this conclusion is based on their density, which is calculated from comparing their size and mass.

Don't expect to find fish in the global oceans. They are probably too warm and under very high pressure, and so there's no such thing as a discrete boundary between the ocean surface and planet atmosphere.

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