Astronomers have unveiled the first 3D model of a planet orbiting a binary system: ScienceAlert

Even today, 5084 exoplanet It has been confirmed in 3,811 planetary systems, while another 8,912 candidates are awaiting confirmation.

These discoveries have provided astronomers with detailed sampling of the types of planets that exist in our universe, ranging from gas giants many times the size of planets. Jupiter into smaller rocky bodies such as the Earth.

So far, the vast majority of these have been discovered using indirect methods – such as transit method (transient photometry) and Radial velocity method (Doppler spectroscopy) – while the rest were detected using various other methods.

In a recent study, an international team of astronomers used the National Science Foundation (NSF) The baseline array is too long (VLBA) to discover a Jupiter-like planet orbiting in a binary system (GJ 896AB) located about 20 light-years from Earth.

Artist’s impression of a small star (orange), orbiting a Jupiter-like planet (blue), and with a farther companion star (red). (Sofia Dagnello, NRAO/AUI/NSF)

Using a method known as Astrometry, the team was able to detect this planet by the “oscillation” it makes as it orbits around the two larger stars in the system. Moreover, this method allowed the team to create the first 3D architecture A binary system and a planet orbiting one of its stars.

The research team was led by Salvador Coriel Ramirez, a researcher at the Institute of Astronomy in National Autonomous University of Mexico (UNAM). He was joined by colleagues from UNAM and researchers with Max Planck Institute for Radio Astronomy (MPIFR) and National Radio Astronomy Observatory (NRAO).

The paper describing their research is entitled3D orbital architecture of a binary dwarf and its planetary companion“on September 1 in Astronomical Journal.

The system under study, GJ 896AB, consists of two red dwarf stars orbiting each other. The larger of the two, which orbits a Jupiter-like exoplanet (GJ 896 Ab), has a mass about 44 percent as much as our sun, while the smaller has a mass of about 17 percent.

They are separated by close to the distance between Neptune and the Sun (about 30 AU) and have an orbital period of 229 years. As explained by Coriel in NRAO press releaseThe 3D maps they made could not be achieved using other exoplanet detection methods.

“Since most stars are in binary or multiple systems, being able to understand systems like this one will help us understand planet formation in general,” he said.

Additionally, M-type (red dwarf) stars are the most common in the universe, accounting for about 75 percent of the stars in the Milky Way alone.

These low-mass, faint stars can remain in their main sequence phase for up to 10 trillion years and are notable for supporting smaller, rocky planets – such as Proxima B and D The system of the seven planets TRAPPIST-1.

In their study, Curiel and colleagues combined VLBA data obtained between 2006 and 2011 (and new data obtained in 2020) with observations made on the system between 1941 and 2017.

The accuracy provided by the ten VLBA telescopes across the United States produced extremely accurate measurements of the positions of the stars over time.

They then performed a comprehensive analysis of the data that revealed the stars’ orbital motions and their combined motions through space. This process, whereby the position of the stars and their proper motion are measured, is known as stellar scaling.

Their detailed evaluation of the larger star’s motion showed a slight wobble caused by the star’s gravitational effect, revealing a planet orbiting it. Based on the level of gravitational influence, the team calculated that the planet is a gas giant, roughly twice the mass of Jupiter.

They also decided that it orbits its parent star at a distance slightly less than that VenusFrom the Sun, it has an orbital period of 284 days, and is included approximately 148 degrees from the two stars’ orbits.

“This means that the planet is moving around the main star in the opposite direction to the secondary star around the main star,” said co-author Gisela Ortiz-Lyon, a researcher with UNAM and MPIA.

“This is the first time such a dynamic structure has been observed in a planet associated with a compact binary system presumably formed in the same protoplanetary disk.”

Astrometric technology will be a valuable tool for characterizing more planetary systems, which will benefit from observatories as planned The Next Generation Super Large Matrix (ngVLA).

This massive network will consist of 244 18-meter (59 ft) dishes spread over 8,860 kilometers (5,505 miles), with an additional short-spaced group of 19 6-meter (20 ft) dishes at the telescope’s core.

The improved sensitivity will allow astronomers to discover smaller, rocky planets orbiting near their stars – where “Earth-like” planets are most likely to reside. Happy co-author Joel Sanchez Bermudez of UNAM:

“Further detailed studies of this and similar systems can help us gain important insights into how planets form in binary systems. There are alternative theories about the mechanism of formation, and more data could indicate which one is more likely.”

In particular, current models indicate that such a large planet is unlikely to be a companion to such a small star, so perhaps these models need to be adjusted.”

This article was originally published by universe today. Read the original article.