Time-Series Analysis of Broadband Photometry of Neptune from K2

Jason F. Rowe, Patrick Gaulme, Jack J. Lissauer, Mark S. Marley, Amy A. Simon, Heidi B. Hammel, Victor Silva Aguirre, Thomas Barclay, Othman Benomar, Patrick Boumier, Douglas A. Caldwell, Sarah L. Casewell, William J. Chaplin, Knicole D. Colon, Enrico Corsaro, G. R. Davies, Jonathan J. Fortney, Rafael A. Garcia, John E. Gizis, Michael R. HaasBenoit Mosser, Francois-Xavier Schmider

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We report here on our search for excess power in photometry of Neptune collected by the K2 mission that may be due to intrinsic global oscillations of the planet Neptune. To conduct this search, we developed new methods to correct for instrumental effects such as intrapixel variability and gain variations. We then extracted and analyzed the time-series photometry of Neptune from 49 days of nearly continuous broadband photometry of the planet. We find no evidence of global oscillations and place an upper limit of $\sim$5 ppm at 1000 \uhz\ for the detection of a coherent signal. With an observed cadence of 1-minute and point-to-point scatter less than 0.01\%, the photometric signal is dominated by reflected light from the Sun, which is in turn modulated by atmospheric variability of Neptune at the 2\% level. A change in flux is also observed due to the increasing distance between Neptune and the K2 spacecraft, and solar variability with convection-driven solar p modes present.
Original languageEnglish
Article number149
JournalThe Astronomical Journal
Issue number4
Publication statusPublished - 10 Mar 2017

Bibliographical note

31 pages, 6 figure, accepted for publication in AJ


  • astro-ph.EP
  • astro-ph.IM
  • astro-ph.SR


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