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Writer's pictureAbdul Rehman

Planet Weekly: Marshmallows in Space

Updated: Dec 21, 2024

Marshmallows, those soft, airy delights, have captured our hearts and taste buds for generations. Their light, fluffy texture is a result of a delicate balance of ingredients and preparation. But what if we told you that there are celestial bodies out there, billions of miles away, that share a similar ethereal quality?


Introducing you to Kepler-51b, a super-puffy exoplanet that defies expectations. This bizarre world, located about 2,400 light-years away, is roughly the size of Jupiter but significantly less massive. Its low density and thick atmosphere give it a soft, fluffy, and marshmallow-like appearance.


kepler 51-b
Kepler 51-b

Discovered in 2012 by NASA's Kepler space telescope, Kepler-51b orbits a G-type star similar to our Sun. Its unique characteristics have intrigued astronomers worldwide. The planet's low density is thought to be due to its extended atmosphere, which is primarily composed of hydrogen and helium. This atmosphere, having been constantly bombarded by intense stellar radiation, has expanded significantly, giving the planet its puffy appearance.


While such planets are quite fascinating to discover, the exact mechanisms behind the formation and evolution of super-puffy planets remain a mystery. One theory suggests that these planets may have formed far from their stars and migrated inward, losing much of their mass in the process. Another possibility is that they formed as gas giants but experienced rapid atmospheric loss due to intense stellar radiation.


Despite their intriguing nature, super-puffy planets pose significant challenges for astronomers. Their low density and thick atmospheres make it difficult to study their internal structure and composition. Traditional methods of exoplanet characterization, such as transit photometry and radial velocity measurements, are not always sufficient to unravel the secrets of these enigmatic planets.


However, as technology continues to advance, astronomers are developing new techniques to probe the atmospheres of exoplanets. By analyzing the light that passes through a planet's atmosphere, scientists can identify the chemical elements present and gain insights into its composition and temperature, perhaps even gaining the ability to decipher the exact mechanics of such fluffy planets.


The study of super-puffy planets is just one example of the many exciting discoveries being made in the field of exoplanet science. As we continue to explore the cosmos, we may uncover even more bizarre and wonderful celestial objects. Until then, we can appreciate the cosmic connection between a distant exoplanet and a familiar earthly treat, reminding us that even in the vastness of space, there's always room for a bit of sweetness.

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