mountain profile Institute for Astronomy University of Hawaii

Planets With the Highest Likelihood of Harboring Life Identified

Maintained by RRG

EMBARGOED UNTIL 0800 US Hawaii Time on 3 August 2016


Contacts:


Nader Haghighipour
cell: +1 808-772-1807
nader@ifa.hawaii.edu

Dr. Roy Gal
Media Contact
+1 808-956-6235
cell: +1 301-728-8637
rgal@ifa.hawaii.edu

Versions of artwork:

Hi-res JPG

 

A team of astronomers known as the Kepler Habitable Zone Working Group, including University of Hawai'i Institute for Astronomy astronomer Nader Haghighipour, has identified which of the more than 4,000 exoplanets discovered by the NASA Kepler mission are most likely to be similar to our rocky home.

The research describes 49 Kepler-discovered planets with radii smaller than twice that of Earth (a criterion for the planet to be rocky) located within the habitable zones (HZ) of their host stars - an area around a star where a rocky planet can maintain liquid water on its surface. Of these planets, 20 are excellent candidates for habitable rocky planets similar to Earth. The work is detailed in an article for Astrophysical Journal led by Dr. Stephen Kane from San Francisco University.

"After more than 3 years analyzing Kepler data, we have created the most complete catalog of Kepler Habitable Zone planets, with the largest number of rocky planets that could potentially harbor life," said Haghighipour. The list contains a total of 216 planets with different sizes, some much larger than Earth.


A graphic showing the habitable zone for stars of different temperatures, along with several planetary candidates, confirmed <em>Kepler</em> planets and Solar System planets.

The Habitable Zones around stars with different surface temperatures. The figure also shows an artist's rendering of the planetary candidates and confirmed Kepler planets that are smaller than twice the size of Earth. For comparison, Venus, Earth, and Mars are also shown. The colored curves delineate various possible inner and outer limits for the Habitable Zone. The red and yellow curves, respectively, show inner limits based on the empirical observation that the surface of Venus has been dry for at least a billion years, and the distance at which the oceans evaporate entirely. The blue and orange curves are outer limits, where the CO2 greenhouse effect maximizes (blue), and based on the observation that Mars appears to have been habitable 3.8 billion years ago when the solar luminosity was 25% lower (orange).


The research also confirms that the distribution of Kepler planet sizes within the habitable zone is the same as the distribution of those outside of it. Haghighipour said; "Given that many of these planets are as large as gas-giant planets in our solar system, there is a high possibility that these planets may harbor large moons that could also be habitable." The latter, combined with the similarity between the distribution of planets inside and outside of the HZ presents strong evidence that the universe is teeming with planets and moons where life could potentially exist.

The boundaries of the habitable zone are critical. If a planet is too close to its star, it will experience a runaway greenhouse gas effect, like Venus. But if it's too far, any water will freeze, as is seen on Mars. The team sorted the planets by whether they were in a conservative or a more optimistic interpretation of the habitable zone. Then they further sorted them by planet size: smaller, rocky planets versus larger gas giants.

These categories will help astronomers focus their research. Those looking for moons that could potentially hold life can study exoplanets in the gas giant categories, for example.

The 20 planets in the most restrictive category - rocky surface and a conservative habitable zone - are the most likely to be similar to Earth. "These are the prime targets for our studies with large ground-based telescopes such as the Keck, Subaru and Gemini telescopes - and in the future, the Thirty Meter Telescope," said Haghihgipour.

"A catalog of Kepler habitable zone exoplanet candidates," by Stephen R. Kane, Michelle L. Hill, James F. Kasting, Ravi Kumar Kopparapu, Elisa V. Quintana, Thomas Barclay, Natalie M. Batalha, William J. Borucki, David R. Ciardi, Nader Haghighipour, Natalie R. Hinkel, Lisa Kaltenegger, Franck Selsis and Guillermo Torres, can be read online here and will be published in an upcoming print edition of the Astrophysical Journal.


Founded in 1967, the Institute for Astronomy at the University of Hawaii at Manoa conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakala and Maunakea. The Institute operates facilities on the islands of Oahu, Maui, and Hawaii.