NASA's next planet hunter will look closer to home

NASA’s next planet hunter will look closer to home
TESS will look at the nearest, brightest stars to find planetary candidates that scientists will observe for years to come. Credit: NASA's Goddard Space Flight Center

As the search for life on distant planets heats up, NASA's Transiting Exoplanet Survey Satellite (TESS) is bringing this hunt closer to home. Launching in 2017-2018, TESS will identify planets orbiting the brightest stars just outside our solar system using what's known as the transit method.

When a planet passes in front of, or transits, its parent star, it blocks some of the star's light. TESS searches for these telltale dips in brightness, which can reveal the planet's presence and provide additional information about it.

TESS will be able to learn the sizes of the planets it sees and how long it takes them to complete an orbit. These two pieces of information are critical to understanding whether a planet is capable of supporting life. Nearly all other planet classifications will come from follow up observations, by both TESS team ground telescopes as well as ground- and space-based observations, including NASA's James Webb Space Telescope launching in 2018.

Compared to the Kepler mission, which has searched for exoplanets thousands to tens of thousands of light-years away from Earth towards the constellation Cygnus, TESS will search for exoplanets hundreds of light-years or less in all directions surrounding our solar system.

TESS will survey most of the sky by segmenting it into 26 different segments known as tiles. The spacecraft's powerful cameras will look continuously at each tile for just over 27 days, measuring visible light from the brightest targets every two minutes. TESS will look at stars classified as twelfth apparent magnitude and brighter, some of which are visible to the naked eye. The higher the apparent magnitude, the fainter the star. For comparison, most people can see stars as faint as sixth magnitude in a clear dark sky and the faintest star in the Big Dipper ranks as third magnitude.

Among the stars TESS will observe, small bright are ideal for planet identification, explained Joshua Pepper, co-chair of the TESS Target Selection Working Group. One of the TESS science goals is to find Earth- and super-Earth-sized planets. These are difficult to discover because of their small size compared to their host stars, but focusing TESS on smaller stars makes finding these small planets much easier. This is because the fraction of the host star's light that a planet blocks is proportional to the planet's size.

Scientists expect TESS to observe at least 200,000 stars during the two years of its spaceflight mission, resulting in the discovery of thousands of new exoplanets.

While the search for transiting exoplanets is the primary goal of the mission, TESS will also make observations of other astrophysical objects through the Guest Investigator (GI) Program. Because TESS is conducting a near all-sky survey, it has the capability to perform interesting studies on many different types of astronomical target.

"The goal of the GI Program is to maximize the amount of science that comes out of TESS," said Padi Boyd, director of the Guest Investigator Program Office at NASA's Goddard Space Flight Center. "Although TESS was designed to be capable of detecting planets transiting in front of stars, its unique mission characteristics mean that the potential science TESS can do includes far more than just exoplanets." According to Boyd, the broad range of objects TESS could detect as part of the GI Program include flaring young stars, binary pairs of stars, supernovae in nearby galaxies, and even supermassive black holes in distant active galaxies. "We hope the broader science community will come up with many unique science ideas for TESS, and we hope to encourage broad participation from the larger community," she said.

With the potential to expand our knowledge of the universe for years to come, researchers are excited about the potential discoveries TESS could bring.

"The cool thing about TESS is that one of these days I'll be able to go out in the country with my daughter and point to a star and say 'there's a planet around that one,'" said TESS Project Scientist Stephen Rinehart.

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Jul 28, 2016
From Wiki (YMMV) "About 10% of planets with small orbits have such an alignment, and the fraction decreases for planets with larger orbits. For a planet orbiting a Sun-sized star at 1 AU, the probability of a random alignment producing a transit is 0.47%"

For every one they find, there must be many dozens they'll miss.
Makes you wonder !!

Jul 28, 2016
"The cool thing about TESS is that one of these days I'll be able to go out in the country with my daughter and point to a star and say 'there's a planet around that one,'" said TESS Project Scientist Stephen Rinehart.

Great attitude! Reminds me of Ellie and her father in the movie Contact.

The combination of TESS and the James Webb Space Telescope should make for some excellent science in the near future. Hopefully TESS will find some interesting nearby exoplanets for James Webb to image and analyze spectroscopically. It is not to hard to image the TESS/James Webb combination laying the groundwork for some truly inspirational direct imaging space telescopes like ATLAST. http://www.stsci....e/atlast

Jul 28, 2016
No need to wait for this mission to impress your daughter. There are at least 20 stars that are visible to the naked eye and have exoplanets.

A list is here:

Jul 29, 2016
Yes, planet search is statistical.

This program is still a lot faster than the astrobiology exploration of our own system!

Unfortunately, JWST is a cosmological deep time mission, which is more suited to look at Jupiter atmospheres. With a lot of cost (observation time) it *may* also be used to study one promising target around a nearby M star which it may (or may not) be able to study the atmosphere of, including biosignatures. And the upcoming giant ground telescopes will have similar troubles.

TESS will obviously be vital to narrow down the optimal target for these experiments. But mostly it will complement Kepler and baseline our neighborhood vs Kepler's "planet field", and lay a basis for targeted future space/ground giant telescopes.

Anyway, it is an exciting TESS ... eh ... act.

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