Astronomers uncover mysterious origins of 'super-Earths'

Astronomers uncover mysterious origins of 'super-Earths'
This artist's impression shows the planet orbiting the Sun-like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super-Earths discovered by the HARPS instrument on the 3.6-metre telescope at ESO's La Silla Observatory. This planet is about 3.6 times as massive as the Earth lis at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist. Credit: ESO/M. Kornmesser

Mini-Neptunes and super-Earths up to four times the size of our own are the most common exoplanets orbiting stars beyond our solar system. Until now, super-Earths were thought to be the rocky cores of mini-Neptunes whose gassy atmospheres were blown away. In a new study published in The Astrophysical Journal, astronomers from McGill University show that some of these exoplanets never had gaseous atmospheres to begin with, shedding new light on their mysterious origins.

From observations, we know about 30 to 50 percent of host stars have one or the other, and the two populations appear in about equal proportion. But where did they come from?

One theory is that most exoplanets are born as mini-Neptunes but some are stripped of their by radiation from host stars, leaving behind only a dense, rocky core. This theory predicts that our Galaxy has very few Earth-sized and smaller exoplanets known as Earths and mini-Earths. However, recent observations show this may not be the case.

To find out more, the astronomers used a simulation to track the evolution of these mysterious exoplanets. The model used thermodynamic calculations based on how massive their rocky cores are, how far they are from their host stars, and how hot the surrounding gas is.

"Contrary to previous theories, our study shows that some exoplanets can never build gaseous atmospheres to begin with," says co-author Eve Lee, Assistant Professor in the Department of Physics at McGill University and the McGill Space Institute.

The findings suggest that not all super-Earths are remnants of mini-Neptunes. Rather, the exoplanets were formed by a single distribution of rocks, born in a spinning disk of gas and dust around host stars. "Some of the rocks grew gas shells, while others emerged and remained rocky super-Earths," she says.

Astronomers uncover mysterious origins of 'super-Earths'
This artist's impression shows the planet orbiting the Sun-like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super-Earths discovered by the HARPS instrument on the 3.6-metre telescope at ESO's La Silla Observatory. This planet is about 3.6 times as massive as the Earth lis at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist. Credit: ESO/M. Kornmesser

How mini-Neptunes and super-Earths are born

Planets are thought to form in a spinning disk of gas and dust around . Rocks larger than the moon have enough to attract surrounding gas to form a around its core. Over time this shell of gas cools down and shrinks, creating space for more surrounding gas to be pulled in, and causing the to grow. Once the entire shell cools down to the same temperature as the surrounding nebular gas, the shell can no longer shrink and growth stops.

For smaller cores, this shell is tiny, so they remain rocky exoplanets. The distinction between super-Earths and mini-Neptunes comes about from the ability of these rocks to grow and retain gas shells.

"Our findings help explain the origin of the two populations of exoplanets, and perhaps their prevalence" says Lee. "Using the theory proposed in the study, we could eventually decipher how common rocky exoplanets like Earths and mini-Earths may be."

"Primordial Radius Gap and Potentially Broad Core Mass Distributions of Super-Earths and Sub-Neptunes" by Eve Lee and Nicholas Connors was published in The Astrophysical Journal.


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More information: "Primordial Radius Gap and Potentially Broad Core Mass Distributions of Super-Earths and Sub-Neptunes" Astrophysical Journal (2021). iopscience.iop.org/article/10. … 847/1538-4357/abd6c7
Journal information: Astrophysical Journal

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Citation: Astronomers uncover mysterious origins of 'super-Earths' (2021, February 10) retrieved 20 September 2021 from https://phys.org/news/2021-02-astronomers-uncover-mysterious-super-earths.html
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