Astronomy

Water-World Super-Earth Found in Nearby Binary System

Astronomers using NASA’s Transiting Exoplanet Survey Satellite (TESS) and the SPIRou spectropolarimeter on the 3.6-m Canada-France-Hawaii telescope have discovered a temperate super-Earth exoplanet orbiting a red dwarf in the binary system TOI-1452.

An artistic rendition of the super-Earth TOI-1452b. Image credit: Benoit Gougeon, Université de Montréal.

An artistic rendition of the super-Earth TOI-1452b. Image credit: Benoit Gougeon, Université de Montréal.

The TOI-1452 binary system resides about 100 light-years away in the constellation of Draco.

Also known as TIC 420112589 or 2MASS J19204172+7311434, it consists of two M-dwarf (red dwarf) stars.

The two stars orbit each other once every 1,400 years and are separated by a small distance — 97 AU (astronomical units), or about 2.5 times the distance between the Sun and Pluto.

The newfound planet circles the primary member of the TOI-1452 system in a temperate orbit that takes 11.1 days.

Named TOI-1452b, the alien world is about 1.7 times larger and 4.8 times more massive than Earth.

“The planet is located at a distance from its star where its temperature would be neither too hot nor too cold for liquid water to exist on its surface,” said Université de Montréal Ph.D. student Charles Cadieux and colleagues.

 

TOI-1452b is probably rocky like Earth, but its radius, mass, and density suggest a world very different from our own.

“TOI-1452b is one of the best candidates for an ocean planet that we have found to date,” Cadieux said.

“Its radius and mass suggest a much lower density than what one would expect for a planet that is basically made up of metal and rock, like Earth.”

According to the astronomers, water may make up 22% of TOI-1452b’s mass, a proportion similar to that of Jupiter’s moons Ganymede and Callisto and Saturn’s moons Titan and Enceladus.

“The water world candidate TOI-1452b is a prime target for future atmospheric characterization with the NASA/ESA/CSA James Webb Space Telescope, featuring a transmission spectroscopy metric similar to other well-known temperate small planets such as LHS 1140b and K2-18b,” they said.

“The system is located near Webb’s northern continuous viewing zone, implying that is can be followed at almost any moment of the year.”

source: sci.news

Y M

Related Posts

El sistema solar tendrá un segundo Sol

  La enana naranja Gliese 710 cruzará las fronteras gravitacionales de nuestro sistema solar dentro de unos 1,3 millones de años, según un informe publicado por los investigadores…

Enorme lago de agua helada en Marte facilitará la colonización

Enorme lago de agua helada en Marte facilitará la colonización La revista Geophysical Research Letters acaba de publicar un artículo donde se detalla el descubrimiento de un enorme lago…

Kepler encuentra gemelo de la tierra con una órbita de 395 días y capaz de albergar vida

Un planeta recién descubierto capaz de albergar vida. Science Magazine, New Scientist, ha revelado que se han descubierto 20 mundos extraterrestres que podrían albergar vida. Según un análisis…

All Alone in the Cosmos: A Unique Galaxy Mystifies Astronomers

Astronomers have discovered an unusually lonely galaxy, 3C 297, using NASA’s Chandra X-ray Observatory and the International Gemini Observatory. Located 9.2 billion light-years from Earth, the galaxy appears…

The James Webb Space Telescope found the farthest galaxy ever seen

The James Webb Space Telescope (JWST) is a space telescope that was launched in December 2021 and is currently conducting infrared astronomy. It is the largest optical telescope…

Las dos lunas de Marte en realidad son fragmentos de una luna mayor desaparecida, según un nuevo estudio

Marte tiene dos lunas: Fobos y Deimos, pero no se parecen mucho a nuestro propio satélite. Ambas son pequeñas y tienen una forma tremendamente irregular. Un nuevo estudio aporta pruebas que…

Leave a Reply

Your email address will not be published. Required fields are marked *