Kepler’s last planet discoveries: two new planets and one single-transit candidate from K2 campaign 19

Author:

Incha Elyse12ORCID,Vanderburg Andrew3,Jacobs Tom4ORCID,LaCourse Daryll5,Bieryla Allyson6,Pass Emily6,Howell Steve B7,Berlind Perry6,Calkins Michael6,Esquerdo Gilbert6,Latham David W6,Mann Andrew W8

Affiliation:

1. Department of Astronomy, University of Wisconsin-Madison , 475 N. Charter St., Madison, WI 53703, USA

2. UW-Madison Sophomore Research Fellow and Hilldale Research Fellow , 500 Lincoln Dr., Madison, WI 53706, USA

3. Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology , Cambridge, MA 02139, USA

4. Amateur Astronomer , 12812 SE 69th Place, Bellevue, WA 98006, USA

5. Amateur Astronomer , 7507 52nd Pl NE, Marysville, WA 98270, USA

6. Center for Astrophysics | Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA

7. NASA Ames Research Center , Moffett Field, CA 94035, USA

8. Department of Physics and Astronomy, The University of North Carolina at Chapel Hill , Chapel Hill, NC 27599, USA

Abstract

ABSTRACT The Kepler space telescope was responsible for the discovery of over 2700 confirmed exoplanets, more than half of the total number of exoplanets known today. These discoveries took place during both Kepler’s primary mission, when it spent 4 yr staring at the same part of the sky, and its extended K2 mission, when a mechanical failure forced it to observe different parts of the sky along the ecliptic. At the very end of the mission, when Kepler was exhausting the last of its fuel reserves, it collected a short set of observations known as K2 Campaign 19. So far, no planets have been discovered in this data set because it only yielded about a week of high-quality data. Here, we report some of the last planet discoveries made by Kepler in the Campaign 19 dataset. We conducted a visual search of the week of high-quality Campaign 19 data and identified three possible planet transits. Each planet candidate was originally identified with only one recorded transit, from which we were able to estimate the planets’ radii and estimate the semimajor axes and orbital periods. Analysis of lower-quality data collected after low fuel pressure caused the telescope’s pointing precision to suffer revealed additional transits for two of these candidates, allowing us to statistically validate them as genuine exoplanets. We also tentatively confirm the transits of one planet with TESS. These discoveries demonstrate Kepler’s exoplanet detection power, even when it was literally running on fumes.

Funder

NASA

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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