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

被引:2
|
作者
Incha, Elyse [1 ,2 ]
Vanderburg, Andrew [3 ,4 ]
Jacobs, Tom [5 ]
LaCourse, Daryll [6 ]
Bieryla, Allyson [7 ]
Pass, Emily [7 ]
Howell, Steve B. [8 ]
Berlind, Perry [7 ]
Calkins, Michael [7 ]
Esquerdo, Gilbert [7 ]
Latham, David W. [7 ]
Mann, Andrew W. [9 ]
机构
[1] Univ Wisconsin, Dept Astron, 475 N Charter St, Madison, WI 53703 USA
[2] 500 Lincoln Dr, Madison, WI 53706 USA
[3] MIT, Dept Phys, Cambridge, MA 02139 USA
[4] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
[5] Amateur Astronomer, 12812 SE 69th Pl, Bellevue, WA 98006 USA
[6] Amateur Astronomer, 7507 52nd Pl NE, Marysville, WA 98270 USA
[7] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA
[8] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[9] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
planets and satellites: detection; planetary systems; ZODIACAL EXOPLANETS; ECLIPSING BINARIES; VALIDATED PLANETS; SUPER-EARTHS; MASS; STAR; SYSTEM; LIGHT; III; PARAMETERS;
D O I
10.1093/mnras/stad1049
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:474 / 487
页数:14
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