Topic: Space
Scientists studied an exoplanet called LHS 3844b, which has extreme temperatures due to its unique rotation. They found that life might be possible on this planet because of a stable internal heat circulation.
LHS 3844b is an exoplanet located about 48.5 light years from our solar system. It orbits the red dwarf star LHS 3884 and has a special property called tidal locking, which means it rotates once on its axis in exactly the same amount of time it takes to orbit its star.
This results in one side of the planet always facing the star and experiencing constant daylight, while the other side is in permanent darkness. The daytime temperature can reach up to 2,000 Kelvin, while the night side is almost absolute zero (0 Kelvin).
At first glance, this extreme environment seems inhospitable for life. However, scientists Daisuke Noto and his team from the University of Pennsylvania wanted to explore further.
They built a laboratory model to mimic the interior of LHS 3844b using a tabletop tank filled with glycerol and thermochromic liquid crystals. The experiment revealed a stable internal heat circulation that behaves like a steady planetary heartbeat.
The researchers found that hot material rises beneath the day side, flows across the upper region, cools as it reaches the night side, then sinks before returning through the lower mantle. This creates a continuous circulation loop that is slow and predictable.
Why It Matters
This discovery is important because it shows that life might be possible on planets with extreme temperatures. It also highlights the importance of studying internal heat circulation in understanding planetary habitability.
Key Facts
- LHS 3844b is an exoplanet located about 48.5 light years from our solar system.
- The planet has a special property called tidal locking, which means it rotates once on its axis in exactly the same amount of time it takes to orbit its star.
- The daytime temperature can reach up to 2,000 Kelvin, while the night side is almost absolute zero (0 Kelvin).
- Scientists built a laboratory model to mimic the interior of LHS 3844b using a tabletop tank filled with glycerol and thermochromic liquid crystals.
- The experiment revealed a stable internal heat circulation that behaves like a steady planetary heartbeat.
Key Terms
- Tidal Locking
- A property of an exoplanet where it rotates once on its axis in exactly the same amount of time it takes to orbit its star.
Implications
This discovery is important because it shows that life might be possible on planets with extreme temperatures. It also highlights the importance of studying internal heat circulation in understanding planetary habitability.
Source: https://www.sciencedaily.com/releases/2026/07/260709160657.htm
Journal Reference:
- Daisuke Noto, Takehiro Miyagoshi, Tomomi Terada, Takatoshi Yanagisawa, Yuji Tasaka. Convective dynamics in mantle of tidally-locked exoplanets. Nature Communications, 2025; 16 (1) DOI: 10.1038/s41467-025-62026-z
Leave a Comment