Astronomers discover two “super-Earths” orbiting a nearby star

Astronomers discover two

TESS photometry of LP 890-9. For each of the four sectors, the 2-minute data points (in gray) were divided into 30-minute intervals to generate the black points, with error bars corresponding to the root-mean-square of the uncertainties of the points in trash can. The LP 890-9 b and c transits are indicated by red and blue dotted lines, respectively. The region marked in orange in Sector 4 was affected by thermal effects and was therefore excluded from the analysis. Source: Delrez et al., 2022.

An international team of astronomers report the discovery of two new “super-Earth” exoplanets orbiting a nearby late-type M dwarf star. The newly discovered extraterrestrial worlds, designated LP 890-9 b and LP 890-9 c, are slightly larger than Earth. The finding was published in Astronomy & Astrophysics.

“Super-Earths” are planets that are more massive than Earth but do not exceed the mass of Neptune. Although the term “super-Earth” only refers to the planet’s mass, it is also used by astronomers to describe planets larger than Earth but smaller than the so-called “mini-Neptunes” (with a radius between two and four Earth radii).

Now, astronomers led by Laetitia Delrez of the University of Liège in Belgium have discovered two new super-Earth class planets. They observed LP 890-9 – a nearby M6V spectral type dwarf star – with NASA’s Transiting Exoplanet Survey Satellite (TESS). This led to the discovery of the inner planet, which was given the designation LP 890-9 b. Follow-up observations of this system with the SPECULOOS (Search for habitable Planets EClipsing ULtra-cOOl Stars) Southern Observatory led to the discovery of a second longer period transiting planet – LP 890-9 c.

“We presented the discovery and first characterization of the LP 890-9 system, which hosts two temperate super-Earths passing through a nearby M6 dwarf,” the researchers wrote in the publication.

LP 890-9 b has a radius of about 1.32 Earth radii and its mass is estimated to be no more than 13.2 Earth masses. The planet orbits its host every 2.73 days at a distance of about 0.018 AU from it. The equilibrium temperature of LP 890-9 b was calculated to be 396 K.

For LP 890-9 c, its radius has been measured to be almost 1.37 Earth radii, while its mass is believed to be less than 25.3 Earth masses. The exoplanet is separated from his parent star around 0.04 AU and has a orbital period of about 8.46 days. The planet’s equilibrium temperature is estimated at 272 K.

The host star LP 890-9 has a radius of about 0.15 solar radii and a mass of 0.12 solar masses. The effective temperature of this M dwarf is around 2,871 K and its luminosity is around 0.00143 solar luminosities. The star is at about 104 light years away from the earth.

Summarizing the results, the astronomers stressed that their discovery makes LP 890-9 the second coolest planet-hosting star after TRAPPIST-1. They added that LP 890-9 c is the second-most favorable habitable zone terrestrial planet known to date.

“The discovery of the remarkable LP 890-9 system presented in this work provides another rare opportunity to study temperate terrestrial life planets around our smallest and coolest neighbors,” the authors of the study concluded.

Two planets orbiting a nearby star have been discovered using TESS

More information:
L. Delrez et al., Two temperate super-Earths crossing a nearby late-type M dwarf, Astronomy & Astrophysics (2022). DOI: 10.1051/0004-6361/202244041

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Citation: Astronomers Discover Two “Super-Earths” Orbiting Nearby Stars (2022, September 14) Retrieved September 15, 2022 from -nearby-star.html

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