The Detection of a Possible Exoplanet Orbiting KIC 1718360 Using Machine Learning
This paper presents the detection of a periodic dimming event in the lightcurve of the G1.5IV-V type star KIC 1718360. This is based on visible-light observations conducted by both the TESS and Kepler space telescopes.
Analysis of the data points toward a possible orbiting body with a radius of approximately 1.048 Earth Radii with a period of 2.938 days, as well as a semi-major axis of 0.04 AU. The initial observation was made in Kepler Quarter 16 data using the One-Class SVM machine learning method. Subsequent observations by the TESS space telescope corroborate these findings.
While still requiring further data to validate, these results may contribute to a growing body of data of Earthlike planets with short-period orbits.
Jakob Roche
Comments: 6 pages, 6 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM); Machine Learning (cs.LG)
Cite as: arXiv:2405.05282 [astro-ph.EP] (or arXiv:2405.05282v1 [astro-ph.EP] for this version)
Submission history
From: Jakob Roche
[v1] Tue, 7 May 2024 12:34:18 UTC (233 KB)
https://arxiv.org/abs/2405.05282
Astrobiology,