The ‘Forbidden’ planet has been found in the ‘Neptunian Desert’

IMAGE

Credit: University of Warwick/Mark Garlick

  • A Neptunian planet has been found in what should be a ‘Neptunian Desert’ by telescopes run by the University of Warwick in an international collaboration of astronomers.
  • NGTS-4b is 20% smaller than Neptune, about 3 times the size of Earth, and has been nicknamed the ‘Forbidden’ planet by researchers
  • Discovered using the state-of-the-art Next-Generation Transit Survey (NGTS) observing facility, designed to search for transiting planets on bright stars, but NGTS-4b is so small other ground surveys wouldn’t have spotted it.
  • It’s hotter than Mercury at 1,000 degrees Celsius

An exoplanet smaller than Neptune with its own atmosphere has been discovered in the Neptunian Desert, by an international collaboration of astronomers, with the University of Warwick taking a leading role.

New research, led by Dr Richard West including Professor Peter Wheatley, Dr Daniel Bayliss and Dr James McCormac from the Astronomy and Astrophysics Group at the University of Warwick, has identified a rogue planet.

NGTS is situated at the European Southern Observatory’s Paranal Observatory in the heart of the Atacama Desert, Chile. It is a collaboration between UK Universities Warwick, Leicester, Cambridge, and Queen’s University Belfast, together with Observatoire de Genève, DLR Berlin and Universidad de Chile.

NGTS-4b, also nick-named ‘The Forbidden Planet’ by researchers, is a planet smaller than Neptune but three times the size of Earth.

It has a mass of 20 Earth masses, and a radius 20% smaller than Neptune, and is 1000 degrees Celsius. It orbits around the star in only 1.3 days – the equivalent of Earth’s orbit around the sun of one year.

It is the first exoplanet of its kind to have been found in the Neptunian Desert.

The Neptunian Desert is the region close to stars where no Neptune-sized planets are found. This area receives strong irradiation from the star, meaning the planets do not retain their gaseous atmosphere as they evaporate leaving just a rocky core. However NGTS-4b still has its atmosphere of gas.

When looking for new planets astronomers look for a dip in the light of a star – this the planet orbiting it and blocking the light. Usually only dips of 1% and more are picked up by ground-based searches, but the NGTS telescopes can pick up a dip of just 0.2%

Researchers believe the planet may have moved into the Neptunian Desert recently, in the last one million years, or it was very big and the atmosphere is still evaporating.

Dr Richard West, from the Department of Physics at the University of Warwick comments:

“This planet must be tough – it is right in the zone where we expected Neptune-sized planets could not survive. It is truly remarkable that we found a transiting planet via a star dimming by less than 0.2% – this has never been done before by telescopes on the ground, and it was great to find after working on this project for a year.

“We are now scouring out data to see if we can see any more planets in the Neptune Desert – perhaps the desert is greener than was once thought.”

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Notes to Editors:

High-res image available at:

https://warwick.ac.uk/services/communications/medialibrary/images/may2019/exoplanet_ngts-4b_-_v4.jpg

The full paper will be available to view on May 29th at: https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stz1084/5475662

Please contact Alice Scott for a copy of the paper if you need it before at: [email protected]

The project was funded by the participating institutions, and with support from the UK Science and Technology Facilities Council, (grant number ST/M001962/1).

All institutions involved are:

Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK

Dept. of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK

Astrophysics Group, Cavendish Laboratory, J.J. Thomson Avenue, Cambridge CB3 0HE, UK

Observatoire de Gen`eve, Universit´e de Gen`eve, 51 Ch. des Maillettes, 1290 Sauverny, Switzerland

Department of Physics and Astronomy, Leicester Institute of Space and Earth Observation, University of Leicester, LE1 7RH, UK

Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, 12489 Berlin, Germany

Institute of Astronomy, Cambridge University, Madingley Road, Cambridge CB3 0HA, UK

Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile

Centro de Astrof´?sica y Tecnolog´?as Afines (CATA), Casilla 36-D, Santiago, Chile.

Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr. 36, D-10623 Berlin, Germany

Institute of Geological Sciences, FU Berlin, Malteserstr. 74-100, D-12249 Berlin, Germany

Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, BT7 1NN Belfast, UK

Instituto de Astronom´?a, Universidad Cat´olica del Norte, Angamos 06010, 1270709, Antofagasta, Chile

Space sciences, Technologies and Astrophysics Research (STAR) Institute, Universit´e de Li`ege, 4000 Li`ege, Belgium

Space and Astronomy Department, Faculty of Science, King Abdulaziz University, 21589 Jeddah, Saudi Arabia

King Abdullah Centre for Crescent Observations and Astronomy, Makkah Clock, Mecca 24231, Saudi Arabia

Winton Fellow

FOR FURTHER INFORMATION PLEASE CONTACT

Alice Scott

Media Relations Manager – Science

University of Warwick

Tel: +44 (0) 2476 574 255 or +44 (0) 7920 531 221

E-mail: [email protected]

Media Contact
Alice Scott
[email protected]

Related Journal Article

http://dx.doi.org/10.1093/mnras/stz1084

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