Found: Planets Skimming a Star’s Surface

PRJacksonKeplerPicforWeb.preview

Brian Jackson’s study focuses on planetary candidates with orbital periods so close to their host stars that they are nearly skimming the stellar surface. This artist’s conception from the European Southern Observatory depicts the exoplanet Corot-7b, which is so close to its Sun-like host star that it must experience extreme conditions.

A new planet-hunting survey has revealed planetary candidates with orbital periods as short as four hours and so close to their host stars that they are nearly skimming the stellar surface. If confirmed, these candidates would be among the closest planets to their stars discovered so far. Brian Jackson of the Carnegie Institution for Science’s Department of Terrestrial Magnetism presented his team’s findings, which are based on data from NASA’s Kepler mission, at the American Astronomical Society’s Division of Planetary Sciences meeting Tuesday.

Most gas giant exoplanets with orbital periods less than or equal to a few days are unstable. This is due to decay in their orbits caused by the effects of their star’s proximity. For rocky or icy planets, this disruption could bring them close enough to the star that the force of their own gravity can no longer hold them together in the face of the star’s gravity.

Motivated by these considerations, Jackson’s team conducted a search for very short-period transiting objects in the publicly available Kepler dataset. Their preliminary survey revealed about a half dozen planetary candidates, all with periods less than 12 hours. Even with masses of only a few times that of Earth, the short periods mean they might be detectable by currently operating ground-based facilities.

If confirmed, these planets would be among the shortest-period planets ever discovered, and if common, such planets would be particularly amenable to discovery by the planned TESS mission, which will look for, among other things, short-period rocky planets.

In his presentation, Jackson described the survey, what has been learned about the candidates from Kepler data, and the team’s plans for follow-up observations.

The team includes Carnegie’s Christopher Stark and Alan Boss, as well as Elisabeth Adams of the Planetary Science Institute, Michael Endl of the McDonald Observatory, Phil Arras of the University of Virginia, and Drake Deming of the University of Maryland at College Park.

 

Funding for this work was provided by the Carnegie Institution for Science’s Department of Terrestrial Magnetism.

 

Carnegie Institution for ScienceAbout: Carnegie Institution for Science (8 Posts)

Carnegie investigators are leaders in the fields of plant biology, developmental biology, Earth and planetary sciences, astronomy, and global ecology. The institution has six research departments: the Geophysical Laboratory and the Department of Terrestrial Magnetism, both located in Washington, D.C.; The Observatories, in Pasadena, California, and Chile; the Department of Plant Biology and the Department of Global Ecology, in Stanford, California; and the Department of Embryology, in Baltimore, Maryland.


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2 Comments on "Found: Planets Skimming a Star’s Surface"

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  1. Ryan DeClue says:

    Puts the brakes on the idea that the old Sol will absolutely destroy Earth.

  2. A cosmic waste of time and money what with Kids starving.

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