Mini‑Neptunes are common exoplanets a little smaller than Neptune. They combine rock and metal with thick envelopes of hydrogen, helium and possibly water. Because they appear often around other stars but not in our solar system, astronomers want to know what their surfaces are like.
The new study, led by Professor Eliza Kempton at the University of Chicago, used telescope observations and computer models to re‑examine previous ideas. Observations from the James Webb Space Telescope of the planet GJ 1214 b, which orbits a star in the constellation Ophiucus, suggest its atmosphere may contain larger molecules than simple hydrogen and helium. A heavier atmosphere produces much more weight over the surface and so much higher pressure.
The team simulated planets with different atmospheres and temperatures and found that high pressure can turn molten rock back into solid rock, much as carbon condenses into diamond deep beneath Earth. They conclude that a substantial portion of mini‑Neptunes once thought to be lava worlds may instead have solid surfaces held down by thick atmospheres. The work appears in Astrophysical Journal Letters.
Difficult words
- exoplanets — planet that orbits a star outside our solar system
- envelopes — thick gas layer around a planet or body
- atmosphere — air and gases around a planet or bodyatmospheres
- molecules — very small unit of a chemical substance
- pressure — force from weight on a surface
- simulated — to make a model or test of something
- condenses — to change gas or molten material to solid
- lava worlds — planet with large surface of molten rock
Tip: hover, focus or tap highlighted words in the article to see quick definitions while you read or listen.
Discussion questions
- If a mini-Neptune has a solid surface under a thick atmosphere, how would that change what scientists want to study about the planet?
- Do you think high pressure environments could allow life forms different from those on Earth? Why or why not?
- Which part of the study would you like to learn more about: telescope observations or computer models? Explain your choice.
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