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Vanderbilt’s role in new planet-finding space mission

by | Posted on Wednesday, May. 1, 2013 — 2:42 PM

exoplanet

Artist conception of exoplanet transiting the face of distant star. (Courtesy of MIT/Kavli Institute for Astrophysics and Space Research)

A team of Vanderbilt astronomers headed by Keivan Stassun will play a key role in the planet-seeking space telescope that NASA has just approved and scheduled for launch in 2017.

The $200 million spacecraft is called the Transiting Exoplanet Survey Satellite (TESS). When it is launched in 2017, TESS will perform the first space-borne all-sky survey for planets circling the brightest stars.

The project is headed by scientists at MIT’s Kavli Institute for Astrophysics and Space Research. Stassun is a co-principal investigator on the project and he and his team will be selecting the specific stars that the project will target in its search for subtle, periodic dips in brightness that occurs when a planet transits across a star’s face.

TESS spacecraft

Artist concept of the TESS spacecraft. (Courtesy of MIT’s Kavli Institute for Astrophysics and Space Research)

“I got involved in 2011 during a sabbatical at MIT,” said Stassun, who is a professor of physics and astronomy at Vanderbilt. “At the time, one of the issues they were struggling with was how to select the most promising stars to search for planets.”

It was a process he had already worked through for KELT, the Kilodegree Extremely Little Telescope: a pair of small, land-based telescopes built and operated by Vanderbilt and Ohio State University that are designed specifically for identifying bright stars with planets. KELT, as will TESS, simultaneously records the light coming from millions of the brightest stars and so faces a similar selection problem. “I was able to tell them that we’ve already addressed the problem. They liked our approach so they invited us to join the mission,” he added.

When it is launched TESS will complement the observations being made by Kepler, NASA’s first mission capable of finding Earth-sized planets around other stars. Kepler was designed to observe much fainter stars than TESS but it is focused on a relatively small portion of the Milky Way galaxy. Three Vanderbilt astronomers, including Stassun, are also members of the Kepler science team. As of last January, Kepler had identified 2,740 candidate planets, which are steadily being confirmed by follow-up observations from other telescopes.

Most of the exoplanets that have been discovered to date are giant planets, like Jupiter. Kepler has discovered a number of smaller exoplanets, closer to the size of Earth. But Kepler has difficulty identifying smaller planets because the stars that it examines tend to be extremely faint, which makes it very difficult to confirm discoveries with ground-based telescopes. TESS, by contrast, is targeting the brightest stars specifically to make it easier to discover Earth-sized planets.

“We will be targeting mainly G-type stars similar to the Sun,” said Stassun. “Not only should concentrating on the brightest stars make it easier to find Earth-like planets, but, once we have found them, it should be possible to use large land-based telescopes to get spectra of the planet’s atmosphere.”

Target star chart

Chart shows the stars that TESS will be targeting in red and those currently being targeted by the Kepler space telescope in blue. (Courtesy of MIT’s Kavli Institute for Astrophysics and Space Research.)

These spectra are important because they could provide information about the chemical make-up of the planetary atmospheres. If certain chemicals, like oxygen and methane, are detected it would be a strong indicator that a planet is capable of supporting life.

“We will also target a small number of red dwarf stars (such as Barnard’s star which was discovered by Vanderbilt’s first astronomer) because these are the stars nearest to us. If we are to imagine ever traveling to visit another world, it will be a world around one of these red dwarf neighbors,” Stassun said.

Contact:
David Salisbury, (615) 322-NEWS
david.salisbury@vanderbilt.edu


  • Paul Hallelujah

    According to the Decay Theory of Planetary Formation, planets form in a manner analogous to the decay of nuclei. For example, in beta decay, we have an electron ejected from the nucleus. Terrestrial worlds may fall into this category. In alpha decay, a helium atom is ejected from the nucleus, which gives us gas giants. In all cases, there is an accompanying tell, a burst of radiation (e.g., gamma burst).

    Were the planets thus formed to be found to be accompanied by a radiation burst, one might thereafter look for a new wobble in the parent star, or transit events.

    The Decay Theory of Planetary Formation is superior to the Nebular Hypothesis, in that it allows perfectly for, and explains the existence of gas giants which have been found to inhabit areas close their parent stars.

    Write to me at paulmichael@gmail.com to discuss this theory further. It will greatly increase our understanding of the universe in general, of symmetry in nature, and of exoplanets in particular.

  • http://www.facebook.com/profile.php?id=1188723836 Fred Farzan Namen

    it’s an awesome research and discovery. good luck

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