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Is There a Planet in Another Galaxy?

Published in Extragalactic Planet Candidate 2 mins read

Yes, scientists have identified a strong candidate for a planet located outside our Milky Way galaxy.

The Discovery of M51-ULS-1b

The search for planets beyond our own galaxy has yielded a significant discovery: M51-ULS-1b. This celestial body is considered the first known extragalactic planet candidate, offering compelling evidence that planets can exist in other galaxies. Its discovery was announced in October 2021, following research published in the journal Nature.

What is an Extragalactic Planet?

An extragalactic planet is, simply put, a planet that resides outside our home galaxy, the Milky Way. While thousands of exoplanets (planets outside our solar system) have been confirmed within the Milky Way, finding one in another galaxy is a much more complex endeavor due to the immense distances involved. The detection of M51-ULS-1b marks a pivotal moment in understanding the prevalence of planets across the universe.

Key Characteristics of M51-ULS-1b

M51-ULS-1b is located in the Whirlpool Galaxy, also known as Messier 51 (M51). Its characteristics, as currently understood, provide a glimpse into the nature of planets beyond our galactic neighborhood.

Characteristic Detail
Name M51-ULS-1b
Location Whirlpool Galaxy (M51)
Estimated Size Approximately 0.7 Jupiter Radii (around 50,000 kilometers in radius)
Orbital Distance Estimated to be tens of Astronomical Units (AU)
Status First known extragalactic planet candidate
Discovery Date Published in October 2021

This planet candidate was detected using a unique method that involved observing a dip in X-ray brightness from a binary system within M51. This method is particularly useful for distant objects as X-rays can be more easily observed over vast cosmic distances than visible light.

While M51-ULS-1b is currently a candidate, and further observations are needed for definitive confirmation, its discovery represents a monumental step forward in our quest to understand the distribution of planetary systems throughout the cosmos. It suggests that planets may be a common feature of galaxies beyond our own.