Researchers at two astronomical institutions have, together, discovered two new Earth-like planets orbiting a star relatively close to the sun
Alejandro Suárez Mascareño, an Instituto de Astrofisica de Canarias astronomer, who is the first author of the study, said: “Nature seems bent on showing us that Earth-like planets are very common. With these two we now know seven in planetary systems quite near to the Sun.”.
The newly discovered planets orbit the star GJ 1002, which is at a distance of less than 16 light years from the solar system. Both of them have masses similar to that of the Earth, and they are in the habitability zone of their star.
GJ 1002b, the inner of the two, takes little more than ten days to complete an orbit around the star, while GJ 1002c needs a little over 21 days.
IAC researcher Vera María Passegger, a co-author of the article, added: “GJ 1002 is a red dwarf star, with barely one-eighth the mass of the sun. It is quite a cool, faint star. This means that its habitability zone is very close to the star.”
The proximity of the star to our solar system implies that the two planets, especially GJ 1002c, are excellent candidates for the characterisation of their atmospheres based either on their reflected light, or on their thermal emission.
presence of oxygen
Article co-author Jonay I. González Hernández, who is also an IAC astronomer, said: “The future ANDES spectrograph for the ELT telescope at ESO in which the IAC is participating, could study the presence of oxygen in the atmosphere of GJ 1002c.”
In addition, both planets satisfy the characteristics needed for them to be objectives for the future LIFE mission, which is presently in a study phase.
The discovery was made during a collaboration between the consortia of the two instruments ESPRESSO and CARMENES. GJ 1002 was observed by CARMENES between 2017 and 2019, and by ESPRESSO between 2019 and 2021.
Ignasi Ribas, an astronomer at the Institute of Space Sciences (ICE-CSIC) and director of the Institut d’Estudis Espacials de Catalunya (IEEC), explained: “Because of its low temperature, the visible light from GJ 1002 is too faint to measure its variations in velocity with the majority of spectrographs.”
CARMENES has a sensitivity over a wide range of near-infrared wavelengths which is superior to those of other spectrographs aimed at detecting variations in the velocities of stars, and this allowed it to study GJ 1002, from the 3.5m telescope at Calar Alto observatory.
The combination of ESPRESSO, and the light-gathering power of the VLT 8m telescopes at ESO allowed measurements to be made with an accuracy of only 30cm/ sec, not attainable with any other instrument in the world.
Suárez Mascareño concluded: “Either of the two groups would have had many difficulties if they had tackled this work independently. Jointly we have been able to get much further than we would have done acting independently.”
The study is published in Astronomy & Astrophysics.
Image: Artist’s impression of two Earth-mass planets orbiting the star GJ 1002. © Alejandro Suárez Mascareño and Inés Bonet (IAC).