The James Webb Space Telescope has spotted an exoplanet called HD 3167 b, a lava exoplanet that is so close to its star it should have lost its atmosphere—yet it hasn't. This surprising discovery offers a rare window into how rocky planets, including Earth, might hold onto their air.
Located 154 light-years away, HD 3167 b is a super-Earth covered in molten rock. It orbits its star in about one Earth day, making it one of the most extreme worlds known. But what makes it truly unusual is that it appears to have an atmosphere, contrary to all expectations.
What Is HD 3167 b and Why Is It Called a Cold Lava Planet?
HD 3167 b is a rocky super-Earth, slightly larger than our planet, with a surface likely covered in lava. It sits extremely close to its host star, completing an orbit in just one Earth day. Because of this proximity, it receives intense stellar radiation and winds that should strip away any atmosphere.
Yet observations with the MIRI instrument on the James Webb Space Telescope show signs that the planet retains an atmosphere. This atmosphere helps keep the planet cooler than other lava worlds, earning it the nickname "cold lava planet." The finding challenges our understanding of how atmospheres survive on close-in rocky planets.
Why Is This Discovery So Improbable?
Planets that orbit very close to their stars face extreme conditions. Stellar winds and high-energy radiation are powerful enough to erode and blow away any gaseous envelope. For a planet like HD 3167 b, scientists expected a bare rock, not an atmosphere.
The fact that Webb detected an atmosphere suggests that some mechanism is replenishing or protecting it. Perhaps the lava surface releases gases that continuously form a new atmosphere, or the planet's magnetic field shields it. Either way, this is a puzzle that could reshape our models of planetary evolution.
How Does This Help Us Understand Earth?
Earth is also a rocky planet, and according to most hypotheses, it was once covered in lava during its early history. Studying HD 3167 b gives us a glimpse into what early Earth might have been like and how it could have retained an atmosphere despite harsh conditions. Context on how this played out before sits in James Webb Finds Cold Lava Exoplanet HD 3167 b With Atmosphere.
By observing this distant world, scientists can test theories about atmospheric formation and survival on rocky planets. This, in turn, helps us understand the conditions that made Earth habitable and the factors that could make other planets habitable—or not. The background to this story is set out in Science: latest articles. A related thread runs through NASA's PRIMA Telescope to Fill James Webb's Far-Infrared Gap.
What Instrument Made This Discovery Possible?
The discovery relied on the Mid-Infrared Instrument (MIRI) aboard the James Webb Space Telescope. MIRI is designed to observe in the mid-infrared, where the thermal emission of the planet's atmosphere can be detected. Its sensitivity allowed scientists to measure the faint signal of HD 3167 b's atmosphere against the glare of its star. Earlier coverage in James Webb Telescope Detects Mysterious Signal in Fornax shows how the argument developed. A closer look at the same subject appears in Cosmic Dawn Simulation: MEGATRON Reveals Milky Way Birth.
Webb's suite of instruments continues to push the boundaries of exoplanet science. With each new observation, we learn more about the diversity of worlds in our galaxy and the processes that shape them. Anyone following the wider picture can start with Astronomers Detect Most Distant Fast Radio Burst From Far Galaxy. The same theme surfaces in Hydrogen Fuel Cell Powers NASA Lunar Missions Through Two-Week Nights, which takes a different angle.
Key Takeaways
- HD 3167 b is a lava-covered super-Earth that orbits its star in about one Earth day.
- Despite extreme conditions, it appears to have an atmosphere, as detected by the James Webb Space Telescope's MIRI instrument.
- This atmosphere helps keep the planet cooler than other lava worlds, earning it the nickname "cold lava planet."
- Studying HD 3167 b provides insights into how early Earth might have retained its atmosphere.
- The discovery challenges our understanding of atmospheric survival on close-in rocky planets.
Comparison of Lava Exoplanets
| Planet | Distance from Star | Orbital Period | Atmosphere | Notable Feature |
|---|---|---|---|---|
| HD 3167 b | Very close | ~1 Earth day | Likely present | Cold lava planet, atmosphere detected by Webb |
| 55 Cancri e | Very close | ~0.7 Earth days | Possible | Lava world with potential atmosphere |
| Kepler-10b | Very close | ~0.8 Earth days | None detected | Rocky, no atmosphere |
FAQ
What is HD 3167 b?
HD 3167 b is a super-Earth exoplanet located 154 light-years away. It is a rocky planet covered in lava and orbits its star in about one Earth day. Recent observations suggest it has an atmosphere, which is unusual for such a close-in planet.
Why is it called a cold lava planet?
It is called a cold lava planet because its atmosphere helps keep it cooler than other lava worlds, despite being extremely close to its star. The atmosphere likely redistributes heat or reflects radiation, lowering the planet's overall temperature.
How was the atmosphere detected?
The atmosphere was detected using the MIRI instrument on the James Webb Space Telescope. MIRI observed the planet's thermal emission, revealing signs of an atmosphere that survived the harsh stellar environment.
What does this mean for understanding Earth?
Studying HD 3167 b helps scientists understand how rocky planets, including early Earth, could retain atmospheres despite extreme conditions. It provides clues about the processes that shaped our planet's habitability.