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Secondary eclipse and day-night modulation of exoplanets observed by transiting exoplanet survey satellite
- 1 Chongqi Bashu Secondary School
* Author to whom correspondence should be addressed.
Abstract
Astronomers have identified over five thousand extrasolar planets since the discovery of the first solar-like star in 1995. These systems exhibit greater diversity than our solar system, providing insights into their formation and evolution. To understand these exoplanets and their habitability, it is crucial to examine their atmosphere composition. The Transiting Exoplanet Survey Satellite (TESS) can detect reflected light from exoplanets with high accuracy, providing valuable insights into their formation and potential for life in the Universe. Planetary reflection can be detected by monitoring the light curve, which is the sum of stellar flux and planetary reflection. Orbiting planets may also reveal their presence by modulating reflected starlight, showing day-night variations in observers’ sight lines. However, these flux variations are extremely small, at a level of 0.01%, making detection difficult. This study developed an efficient Python program to search for secondary eclipse and day-night modulation on the TESS light curves of over four hundred known short-period transiting exoplanets. The program automatically identifies and rejects low-quality photometric data points in light curves, folding high-quality light curves in the orbital phase determined by primary transits. The phase-folded average light curves have high photometric precision, suitable for detecting secondary eclipse and day-night modulation. The program successfully identified planetary reflection in seventeen transiting exoplanetary systems, larger than the current TESS sample by twice. The program plans to upgrade to search for orbital phase modulation in non-transit exoplanets, taking advantage of the high precision of TESS photometry.
Keywords
Exoplanets, Photometry, Python
[1]. The Royal Swedish Academy of Sciences. 2019, Scientific Background on the Nobel Prize in Physics 2019
[2]. Mayor, M., & Queloz, D. 1995, Nature, 378, 6555
[3]. Perryman, M. 2018, The Exoplanet Handbook by Michael Perryman, Cambridge University Press, Second Edition
[4]. Kaisey, M. & Agol, E. 2002, ApJ, 580, 171
[5]. Wong, I., et al. 2019, The Astronomical Journal, 159, 104
[6]. Vanderspeck, R., et al. 2018, TESS Instrument Handbook
[7]. Twichen, J. D., et al. 2020, TESS Science Data Products Description Document
[8]. Guerrero, N. M., et al. 2021, ApJS, 254, 39
[9]. Yee, S. W., Winn, J. N., Knutson, H. A., et al. 2020, ApJL, 888, L5
[10]. Wong, I., et al. 2020, The Astronomical Journal, 160, 155
[11]. Wong, I., et al. 2021, The Astronomical Journal, 162, 127
Cite this article
Ye,H. (2024). Secondary eclipse and day-night modulation of exoplanets observed by transiting exoplanet survey satellite. Theoretical and Natural Science,34,229-249.
Data availability
The datasets used and/or analyzed during the current study will be available from the authors upon reasonable request.
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Volume title: Proceedings of the 3rd International Conference on Computing Innovation and Applied Physics
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