UNSW - Science

New neighbours? Closest single Sun-like star may have habitable planet

Wednesday, 19 December, 2012
Bob Beale
Artist's impression of Tau Ceti and planets. (Credit: J. Pinfield for the RoPACS network at the University of Hertfordshire, 2012).

One of the closest stars to Earth, Tau Ceti, may host five planets - with one in the star’s habitable zone  - an international team of astronomers has discovered.

Only 12 light years away, Tau Ceti is the closest single star that  astronomers consider to be like our Sun. It is visible with the naked eye in the evening sky in the constellation Cetus and is currently almost directly overhead after sunset in the Australian sky.

It appears to have five planets estimated to have masses between two and six times the mass of the Earth – making it the lowest-mass planetary system yet detected, the researchers report in a paper published in the journal Astronomy and Astrophysics.

One of the planets lies in the habitable zone of the star and has a mass about five times that of Earth, making it the smallest known planet orbiting in the habitable zone of any Sun-like star.

The international team of astronomers, from the UK, Chile, the USA, and Australia, combined more than 6,000 observations from three different instruments and intensively modelled the data. Using new techniques, the team has found a method to detect signals half the size previously thought possible. They say this greatly improves the sensitivity of searches for small planets and suggests that Tau Ceti is not a lone star but has a planetary system.

"The evidence for planets in this system is certainly tantalising”, says Professor Chris Tinney, an astronomer who leads the Exoplanetary Science at UNSW group and is one of six UNSW authors on the paper. Researchers from the Australian Astronomical Observatory and the University of Southern Queensland were also involved.

“It’s certainly a very exciting prospect to gaze into the night sky and see with your own eyes a star so nearby that may host a habitable planet,” says Tinney. “When you consider the vastness of space, they don’t come much closer than this.”

Tau Ceti has featured prominently in science fiction over many years, including the Star Trek series, Dr Who and numerous computer games. In the 1954 novel Caves of Steel, author Isaac Asimov depicted Tau Ceti as humanity’s first settlement place beyond the solar system.

The first author of the paper, Mikko Tuomi, of the University of Hertfordshire, says the study pioneered new data modelling techniques that have significantly improved noise-modelling techniques and increased the ability to find low-mass planets.

The researchers say  Tau Ceti is so bright and similar to our Sun that it is an ideal benchmark system to test out the new method for the detecting small planets. Its closeness means it may be possible to study the atmospheres of its planets in the future.

Over 800 planets have been discovered orbiting other worlds, but planets in orbit around the nearest Sun-like stars are particularly valuable. Steve Vogt from University of California Santa Cruz said: "This discovery is in keeping with our emerging view that virtually every star has planets, and that the galaxy must have many such potentially habitable Earth-sized planets. They are everywhere, even right next door.”

Australian media contacts:

Chris Tinney (UNSW)  c.tinney@unsw.edu.au; Simon O’Toole (AAO) – otoole@aao.gov.au; Brad Carter (USQ) carterb@usq.edu.au

 

Personnel and funding:

The international research team consists of:

 

• Mikko Tuomi, Hugh Jones, John Barnes and David Pinfield (University of Hertfordshire)

are supported by RoPACS (Rocky Planets Around Cool Stars), which is a Marie Curie

Initial Training Network funded by the European Commissions Seventh Framework

Programme.

• James Jenkins is based at the University of Chile and is a Visiting Fellow at the

University of Hertfordshire.

• Chris Tinney, Rob Wittenmyer, Jonathan Horner, Jeremy Bailey, Duncan Wright and

Graeme Salter (University of New South Wales, Australia) are supported by grants from

the Australian Research Council.

• Steve Vogt from University of California Santa Cruz acknowledges support from NSF

grant AST-0307493

• Paul Butler is supported by the Carnegie Institution for Science.

• Simon O'Toole is supported by the Australian Astronomical Observatory.

• Brad Carter is supported by the University of Southern Queensland

The result is based on spectra from taken as part of the Anglo-Australian Planet Search with the

UCLES spectrograph on the Anglo-Australian Telescope, HIRES on the Keck Telescope and

reanalysis of spectra taken with the HARPS spectrograph and available through the European

Southern Observatory public archive.