Earth-like planet spotted beyond solar system


Astronomers have discovered the most Earth-like planet outside our Solar System to date, an exoplanet with a radius only 50% larger than the Earth and capable of having liquid water. Using the ESO 3.6-m telescope, a team of Swiss, French and Portuguese scientists discovered a super-Earth about 5 times the mass of the Earth that orbits a red dwarf, already known to harbour a Neptune-mass planet. The astronomers have also strong evidence for the presence of a third planet with a mass about 8 Earth masses.

This exoplanet – as astronomers call planets around a star other than the Sun – is the smallest ever found up to now [1] and it completes a full orbit in 13 days. It is 14 times closer to its star than the Earth is from the Sun. However, given that its host star, the red dwarf Gliese 581 [2], is smaller and colder than the Sun – and thus less luminous – the planet nevertheless lies in the habitable zone, the region around a star where water could be liquid!

“We have estimated that the mean temperature of this super-Earth lies between 0 and 40 degrees Celsius, and water would thus be liquid,” explains Stéphane Udry, from the Geneva Observatory (Switzerland) and lead-author of the paper reporting the result. “Moreover, its radius should be only 1.5 times the Earth’s radius, and models predict that the planet should be either rocky – like our Earth – or covered with oceans,” he adds.

“Liquid water is critical to life as we know it,” avows Xavier Delfosse, a member of the team from Grenoble University (France). “Because of its temperature and relative proximity, this planet will most probably be a very important target of the future space missions dedicated to the search for extra-terrestrial life. On the treasure map of the Universe, one would be tempted to mark this planet with an X.”

The host star, Gliese 581, is among the 100 closest stars to us, located only 20.5 light-years away in the constellation Libra (“the Scales”). It has a mass of only one third the mass of the Sun. Such red dwarfs are intrinsically at least 50 times fainter than the Sun and are the most common stars in our Galaxy: among the 100 closest stars to the Sun, 80 belong to this class.

“Red dwarfs are ideal targets for the search for low-mass planets where water could be liquid. Because such dwarfs emit less light, the habitable zone is much closer to them than it is around the Sun,” emphasizes Xavier Bonfils, a co-worker from Lisbon University. Planets lying in this zone are then more easily detected with the radial-velocity method [3], the most successful in detecting exoplanets.

Two years ago, the same team of astronomers already found a planet around Gliese 581 (see ESO 30/05). With a mass of 15 Earth-masses, i.e. similar to that of Neptune, it orbits its host star in 5.4 days. At the time, the astronomers had already seen hints of another planet. They therefore obtained a new set of measurements and found the new super-Earth, but also clear indications for another one, an 8 Earth-mass planet completing an orbit in 84 days. The planetary system surrounding Gliese 581 contains thus no fewer than 3 planets of 15 Earth masses or less, and as such is a quite remarkable system.

The discovery was made thanks to HARPS (High Accuracy Radial Velocity for Planetary Searcher), perhaps the most precise spectrograph in the world. Located on the ESO 3.6-m telescope at La Silla, Chile, HARPS is able to measure velocities with a precision better than one metre per second (or 3.6 km/h)! HARPS is one of the most successful instruments for detecting exoplanets and holds already several recent records, including the discovery of another ‘Trio of Neptunes’ (ESO 18/06, see also ESO 22/04).

The detected velocity variations are between 2 and 3 metres per second, corresponding to about 9 km/h! That’s the speed of a person walking briskly. Such tiny signals could not have been distinguished from ‘simple noise’ by most of today’s available spectrographs.

“HARPS is a unique planet hunting machine,” says Michel Mayor, from Geneva Observatory, and HARPS Principal Investigator. “Given the incredible precision of HARPS, we have focused our effort on low-mass planets. And we can say without doubt that HARPS has been very successful: out of the 13 known planets with a mass below 20 Earth masses, 11 were discovered with HARPS!”

HARPS is also very efficient in finding planetary systems, where tiny signals have to be uncovered. The two systems known to have three low mass planets – HD 69830 and Gl 581 – were discovered by HARPS.

“And we are confident that, given the results obtained so far, finding a planet with the mass of the Earth around a red dwarf is within reach,” affirms Mayor.

Source European Southern Observatory


2 Responses to Earth-like planet spotted beyond solar system

  1. Vishyar April 25, 2007 at 1:52 pm #

    “How do scientists then postulate what a planet may be made of (gassy, rocky, etc.)? What direct evidence is there that the planet contains water, is there any or is this a publicity announcement? What degree of confidence are these proclamations made? How much of these declarations are based on real science and how much is based on theories dependent on theories which themselves are dependent on theories (and so on) which really becomes wishful thinking.”

    Doug,
    Those (tentative) conclusions are based on the areas where rocky planets vs. gassy ones tend to form, and the size that they tend to take. Gas giants usually have to be big, because of issues with gravity to keep them together. A gas planet will usually in some way occult its parent star, and may even be visible in some spectra. If no gas giant is seen, it’s likely that the planet is much smaller and rocky. Also, gas giants tend to form far away, because of the way gas and dust distribute during solar system formation.

    You know all those missions to find out what planets are made of, and look at how dust forms around the Sun? Well, the whole point of those is to find out why, and how different planets end up where they do – so that when we look at other solar systems, we have enough information to come to well-educated conclusions.

  2. Doug April 25, 2007 at 10:45 am #

    This is interesting to me but not being a scientist let alone an astrophysicist, there are a few things I don’t understand.

    I can see how detecting a “wobble” would lead to the identification of a planet. It also still seems reasonable that they might be able to pinpoint a location and I guess its not too far beyond that to reason that scientists might be able to estimate the mass of planet and its distance from the star. I’m thinking the speed of the wobble might suggest how fast the orbit is and the degree of the wobble gives clues to the mass of the planet. Are assumptions made about the speed of the planet, to then estimate its distance from its “sun”? If so couldn’t a faster planet provide for a planet of greater mass and a further distance? In any case this all still seems pretty reasonable.

    Here’s where the theoretical leaps seem pretty large. How do scientists then postulate what a planet may be made of (gassy, rocky, etc.)? What direct evidence is there that the planet contains water, is there any or is this a publicity announcement? What degree of confidence are these proclamations made? How much of these declarations are based on real science and how much is based on theories dependent on theories which themselves are dependent on theories (and so on) which really becomes wishful thinking.

    I guess I’m really looking for the real article that actually supports a headline like “Scientists find habitable planet with Liquid Water” hopefully still written such that a laymen can make some sense of it.

    Thanks!!

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