We May absorb Just Found the First Moon external Our Solar System

In Brief

The first moon external of our solar system may absorb been recently detected near the star Kepler-1625 by a team using the Kepler space telescope. While scientists remain cautious in confirming this discovery, it potentially has delightful consequences.

Our First Exomoon?

A sign has been detected by the Kepler Space Telescope that may well be the first moon we absorb ever discovered external of our solar system. It was picked up by David Kipping and his colleagues at Columbia University, who remain speculative. Kipping told modern Scientist, “It is consistent with the sign that we might expect from a moon, but it might be consistent with other things as well.”

Kepler finds cosmic bodies by measuring their disruption of light as they cross the path between us and distant stars. The team detected the dips that indicated the moon over three orbits of a planet in the star system called “Kepler-1625.” They graded the exomoon’s likelihood at four sigma — which means that the probability of seeing the same data whether the moon did not exist is roughly one in 16,000.

However, whether it is indeed a moon, it would be a cosmic anomaly, as the team states that it is roughly the size of Neptune and orbiting a planet the size of Jupiter. On the other hand, as David Waltham at the University of London, said to modern Scientist, “It would be pretty odd that there are hundreds of moons in the solar system but not anything anywhere else.”

Also, it may be that the first exomoons we detect will absorb to be relatively large ones, as smaller moons will likely cause blips in the data that are too small for us to detect yet. In this case, we are attempting to distinguish patterns in the faint light from a star that is 4,000 light-years absent.

A dwelling to Call domestic?

The discovery of an exomoon is exciting because “habitable exomoons could be even more many than soil-analogue exoplanets themselves,” Helmut Lammer argues in a paper published in Origins of Life and Evolution of the Biosphere. This is for two main reasons.

The first reason is that “the majority of confirmed exoplanets and candidates orbiting in the habitable zone (HZ) of their host stars are either super-Earths or gas giants.” Essentially, because our instruments are not precise enough, the huge majority of exoplanets we absorb discovered so far are inhabitable due to their size, which Kepping asserts in a paper would absorb to be twice as massive as Mars for us to even see them. This causes them to absorb gassy and toxic atmospheres, or a gravitational pull that would be unsuitable for humans.

Alien Worlds: Meet The Most Remarkable Moons in Our Solar System
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moment, exomoons are tidally locked to their exoplanets, meaning that their days should be shorter than their stellar years, making them more soil-like and favorable for humans.

The discovery is also meaningful because, whether we can confirm that a moon of this size exists, it vastly expands the horizons of the field. We could start looking specifically for moons of this size and potentially accelerate the discovery of other exomoons.

We won’t know for certain until Hubble is given a chance to gather data on the possible moon. But, whether it is confirmed, this exomoon will be a fabulous discovery that gives us knowledge of the existence of worlds that could be more habitable than exoplanets, as well as enlightening us on another secret of the universe.

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