New planets feature young star and twin Neptunes

Jun 15, 2011
Image: illustration of a system with twin Neptune-like planets.

(PhysOrg.com) -- An international team, including Oxford University scientists, has discovered ten new planets. Amongst them is one orbiting a star perhaps only a few tens of million years old, twin Neptune-sized planets, and a rare Saturn-like world.

The were detected using the CoRoT (, Rotation and Transits) , operated by the French space agency CNES. It discovers planets outside our solar system – exoplanets – when they ‘transit’, that is pass in front of their stars.

The new finds were announced on 14 June at the Second CoRoT Symposium, held in Marseille.

Out of the ten new exoplanets (CoRoT-16b through to 24b and c) seven are hot Jupiters some of which are unusually dense and/or on unusually elongated orbits, and one is in orbit around an unusually young star. The announcement also includes a planet slightly smaller than , and two Neptune-sized planets orbiting the same star.

Dr Suzanne Aigrain of Oxford University’s Department of Physics, lead UK scientist for CoRoT, said: ‘CoRoT-18b is special because its star might be quite young. Finding planets around young stars is particularly interesting because planets evolve very fast initially, before settling into a much steadier pattern of evolution.

‘If we want to understand the conditions in which planets form, we need to catch them within the first few hundred . After that, the memory of the initial conditions is essentially lost. In the case of CoRoT-18, different ways of determining the age give different results, but it's possible that the star might be only a few tens of millions of years old. If this is confirmed, then we could learn a lot about the formation and early evolution of hot gas giant planets by comparing the size of CoRoT-18b to the predictions of theoretical models.’

Another system of particular interest is CoRoT-24, which is around 4,400 light years from us and consists of a star just a little smaller than our Sun, orbited by two transiting planets.

‘The first of these planets is three times larger than the Earth, and takes 5.1 days to orbit the star, whilst the second is 4.8 times larger than the Earth and takes 11.8 days to complete an orbit. So these planets are similar to Neptune in size, but much hotter,’ said Dr Aigrain.

‘However, we don't know yet whether they are also similar to Neptune in composition, because even with the best instruments in the world, we could only obtain upper limits on their masses. It's the first system with two transiting planets found by CoRoT, and it ties in well with similar transiting planet systems found by the Kepler mission.’

Elsewhere CoRoT-22b is a rare example of a planet similar in size to Saturn. Located around 2,000 light years from us it takes about 10 days to orbit its star, which is slightly hotter than our Sun. Dr Aigrain said: ‘we have only an upper limit on its mass, but this is enough to determine that is density is not much more than that of Jupiter, which means it has a predominantly gaseous composition, although it could also contain significant quantities of rock and ice.’

Once CoRoT detects a transit, additional observations are made from the ground, using a number of telescopes all over the world. Although astronomers cannot see the planets directly, they use the space- and ground-based data to measure the sizes, masses, and orbits of these precisely. This is why, among all known exoplanets, those with transits yield the most complete information about planet formation and evolution.

The new planets will also be presented at a seminar on June 15th at the Institute of Physics in London.
 
The 10 new planets are:

CoRoT-16b: A puffed-up short-period giant planet, with half the Jupiter mass and its full radius. It orbits in 5.3 days around a mature Sun-like star with an age of 6 billion years. The orbit of this planet is highly elongated which is rare for such an old, close-in planet.

CoRoT-17b: A massive giant planet around a star with an age of 10 billion years, or twice as old as our Sun. It orbits in 3.7 days, has 2.4 Jupiter masses and a density twice that of Jupiter. Observing such an old planetary system is important for understanding the long term evolution of giant planets.

CoRoT-18b: Unlike the previous CoRoT planets this “Hot Jupiter” orbits a young star that is a mere 600 million years old. This planet has a size 1.4 times that of Jupiter, but 3.5 times its mass. This planet is very dense, with almost twice the density of Jupiter.

CoRoT-19b: A planet with the same mass as Jupiter but 1.5 times the size. It has a density much less than that of Saturn, the least dense planet in our solar system.

CoRoT-20b: A “Hot Jupiter” in an eccentric orbit with a period of 9.2 days. CoRoT-20b is special because it has a very elongated orbit which may be related to its extremely high density. It has a density twice that of Mars, even though it is a gaseous giant planet.

CoRoT-21b: A giant gas planet with a size 1.3 times that of Jupiter and 2.5 times the mass. This is one of the faintest CoRoT stars for which the planet mass has been determined. These mass measurements required observations with the Keck 10m telescope in Hawaii, USA, the largest telescope in the world.

CoRoT-22b: This planet has a size of 0.74 radii that of Saturn. The mass of this exoplanet has yet to be determined precisely, but it is certainly less than half that of Saturn.

CoRoT-23b: A “Hot Jupiter” in a 3.6 day orbit.

CoRoT-24b and 24c: A system with two transiting planets of Neptune size in orbits of 5.1 and 11.8 days. The planets have sizes of 1 and 1.4 times that of , respectively.

Explore further: Exomoons Could Be Abundant Sources Of Habitability

More information: *Despite their best efforts, the team were not able to detect the radial velocity signatures of CoRoT-22b, 24b and 24c unambiguously. However, they were able to rule out almost every configuration of stars that could mimic a planet in the CoRoT data at high confidence.

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Decimatus
5 / 5 (2) Jun 15, 2011
And these are only systems where the planets eclipse their stars in what is a near perfect lineup between that system and the view from earth.

It seems like the rarity lies in a system NOT having planets as opposed to what many have believed for so long.
Starbound
not rated yet Jun 15, 2011
The only problem is that our observation techniques most easily find planets that are horrible, horrible places to live. I wonder when the next data set from Kepler is going to be released?
LKD
1 / 5 (1) Jun 15, 2011
It seems like the rarity lies in a system NOT having planets as opposed to what many have believed for so long.


Pretty much. :) Although binary, triple, quad, etc. star systems will have no planets. There is just no stable orbit in those systems.
gmurphy
not rated yet Jun 15, 2011
The more we discover about other solar systems, the more unusual our own one starts to become, the innermost planet of our solar system takes 243 days to perform a full rotation. Most of the planets we've discovered so far experience orbits around their star of a few weeks or even less. Of course, our data is biased towards detecting these types of solar systems but still impressive.
Decimatus
5 / 5 (1) Jun 16, 2011
Pretty much. :) Although binary, triple, quad, etc. star systems will have no planets. There is just no stable orbit in those systems.


Actually there was a story on here recently about a binary star system with 2 gas giants circling it.

Of course certain types of binary systems will be more or less likely to have planets, but it does happen.

Also, while many stars may not have planets "forever", even a mere billion years with a solar system could potentially be long enough to sustain the evolution of life.

The number of species that may have evolved in the past 10 billion years of milky way history could be quite astounding.
LKD
not rated yet Jun 16, 2011
Actually there was a story on here recently about a binary star system with 2 gas giants circling it.


Yes, I thought that was hysterically appropriate that I would restate about stable orbits around two massive bodies, and there's an exception. :D I wouldn't give the planets long to live, but it is a very amazing system.