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A Star Has Completely Blasted Away the Atmospheric Environment of it's Planet

What would happen if you put an M-dwarf star in a tight orbit around a planet the size of Earth? Given that M dwarfs are the most common stars we are aware of, the question goes beyond mere academic merit. Astronomers researching the planet GJ 1252b have discovered the solution, and it's not nice.


This planet receives a lot of heat because it is so close to its star. Additionally, the closeness is dangerous in another aspect. A planet's atmosphere might be completely destroyed by the star's radiation, according to Michelle Hill, a co-author of new research on GJ 1252b from the University of California, Riverside.

The planet is 65 light years away from Earth and makes two orbits around its star every day. This planet is uninhabitable due to the star's heat.


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In comparison to Mercury in our solar system, this is not all that different. As it rounds the Sun, the planet experiences intermittent heating and freezing because it lacks an atmosphere. In actuality, solar activity also causes a small loss of atmosphere on Earth. But other processes, such as volcanism, release gases back into our atmosphere. Mercury and GJ 1252b are unlucky; Earth is not. And that has important ramifications for the quest for worlds that support life.


Why is M Dwarf Stars special?

In just our galaxy alone, there are billions of M dwarf stars. They are between one-tenth and two-thirds the mass of the Sun in size. These may be active, causing their systems to experience flares and eruptions. In most cases, there is at least one planet within their habitable zones and other planets at various distances.


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If you're hoping to discover life on their planets, that combination is not ideal. Naturally, any hope for life on those worlds is also extinguished by the stellar activity that blasts away their atmospheres. Additionally, the abundance of M dwarfs may reduce the amount of planets in the galaxy that DO host life.


For planets like GJ 1252b, that's not very good news.


According to Hill, "it's possible that the state of this planet could be a terrible sign for planets even further out from this type of star." We'll learn more about this from the James Webb Space Telescope, which will study planets like these.


Even though M dwarfs may destroy the atmosphere, all is not lost. For instance, a large portion of the 5,000 stars in the solar vicinity of Earth are M dwarfs. Even if a significant portion of them manage to make their planets habitable, at least 1,000 more—not all of them M dwarfs—could cultivate environments favorable for life on their planets. "A planet may be able to keep its atmosphere if it is sufficiently far from an M dwarf. We still can't say that Mercury's fate applies to all rocky planets around these stars, Hill added. "I am still hopeful."


On GJ 1252b, looking for an atmosphere

Intriguing science underlies the events at GJ 1252b. Due to a secondary eclipse, which dimmed the planet's light, astronomers utilized data from the Spitzer Space Telescope to estimate its infrared radiation. According to the measurements, the star blasts the planet. The average surface temperature during the day is 1227 C. (2242 F). That is hot enough to cause copper, silver, and gold to melt.


The researchers thought there was no atmosphere because of the heat and low surface pressure they imagined. But suppose for a moment that a carbon dioxide atmosphere DID exist.


This might enable that blanket to last for a while by trapping heat on the surface. GJ 1252b, on the other hand, turns out to be less lucky. "The planet wouldn't have an atmosphere even if it contained 700 times as much carbon as Earth does. Stephen Kane, an astronomer at UC Riverside and a co-author of the paper, stated that it would initially grow up before tapering off and eroding away.


In the long run, the search for habitable planets will shift to alternative candidates orbiting less volatile stars if this study's findings hold true across a sizable population of M dwarf stars.


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