The 2,415th Meeting of the Society

November 1, 2019 at 8:00 PM

Powell Auditorium at the Cosmos Club

TESS’ Exoplanets

Results of the Transiting Exoplanet Survey Satellite Mission

George Ricker

TESS Principal Investigator
Director, CCD Laboratory
MIT Kavli Institute for Astrophysics and Space Research

Sponsored by PSW Science Member Bob Terry

About the Lecture

Successfully launched on a SpaceX Falcon 9 rocket in April 2018, NASA’s Transiting Exoplanet Survey Satellite (TESS) is well on its way to discovering thousands of exoplanets in orbit around the brightest stars in the sky. During its initial two-year survey mission, TESS is monitoring more than 200,000 targeted bright stars in the solar neighborhood for drops in brightness caused by planetary transits. This first-ever space borne all-sky transit survey is identifying planets ranging in size from Earth-sized to gas giants, orbiting a wide variety of host stars, from cool M dwarfs to hot O/B giants.

TESS stars are typically 30 –100 times brighter than those surveyed by the Kepler satellite; thus, TESS planets are proving far easier to characterize with follow-up observations than those from prior missions. Such TESS follow-up observations are enabling measurements of the masses, sizes, densities, orbits, and atmospheres of a large cohort of small planets, including a sample of habitable zone rocky worlds.

An additional data product from the TESS mission is its full frame images (FFIs), which are collected at a cadence of 30 minutes. These FFIs provide precise photometric information for every object within the 2300 square degree instantaneous field of view of the TESS cameras. In total, nearly 100 million objects brighter than magnitude I = +16 will be precisely photometered during TESS’ two-year prime mission.

TESS completed its Southern Ecliptic Hemisphere in July 2019, and is nearing the midway point of its Northern Ecliptic Hemisphere survey. A concurrent, two year-long deep survey by TESS of regions surrounding the North and South Ecliptic Poles will provide prime exoplanet targets for characterization with the James Webb Space Telescope (JWST), as well as other large ground-based and space-based telescopes coming online during the next two decades.

A Guest Investigator program is well underway for TESS, and data download volumes are among the largest of current missions.

The TESS legacy will be a catalog of the nearest and brightest main-sequence stars hosting transiting exoplanets, which should endure as the most favorable targets for detailed future investigations.

TESS received the top science ranking for operating Explorer missions in the just-completed NASA Astrophysics Senior Review, assuring that the mission will be extended through 2022. In principle, TESS’s unique lunar-resonant orbit should facilitate additional extended missions lasting more than a decade.

The status of TESS as it completes its first 1.5 years of survey operations will be reviewed, and information on opportunities for engagement by professional astronomers and amateur members of the public will be discussed as well.

About the Speaker

George R. Ricker is the principal investigator for NASA’s Transiting Exoplanet Sky Survey (TESS) Explorer mission, and Senior Research Scientist and Director of the Detector Laboratory at the MIT Kavli Institute for Astrophysics and Space Research.

George’s current astronomical interests include studies of extrasolar planets, and of transient high energy sources and their counterparts. His experimental research interests are focused on the development of new solid-state photon detectors, based on silicon charged-coupled devices (CCDs) and intended primarily for space astronomy applications.

George also has been a pioneer in the development of small, inexpensive satellites for astronomical missions. He served as Principal Investigator for the international High Energy Transient Explorer (HETE-2) mission, a small satellite incorporating instruments from France, Japan and the United States that operated successfully in orbit for six years. Designed, constructed, and integrated at the MIT Kavli Institute, it was the first satellite mission entirely devoted to the study of gamma-ray bursts.

George has also served as the Principal Investigator for the CCD Solid State Imaging Spectrometer on the Japan-US ASCA mission, which was the first photon-counting CCD instrument ever flown, as Deputy-Principal Investigator for the Advanced CCD Imaging Spectrometer on NASA’s Chandra X-ray Observatory, as the US Principal Investigator for the X-ray Imaging Spectrometer CCD Camera on the Japan-US Astro-E1 mission, and as the MIT Principal Investigator for the suite of silicon-drift detectors for NASA’s Neutron-star Interior Composition Explorer (NICER) mission.

George is an author on more than 300 technical publications.

He earned a BS in Physics at MIT, an MS in astronomy at Yale and a PhD in Physics at MIT.