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Analysis of KOI 2700b, the second exoplanet with a comet-like dusty tail – selected results

Published online by Cambridge University Press:  13 January 2020

Zoltán Garai  and
Peter Dolinský
Zoltán Garai
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, 05960 Tatranská Lomnica, Slovak Republic email: [email protected]
Peter Dolinský
Affiliation:
Slovak Central Observatory, Komárňanská 134, 94701 Hurbanovo, Slovak Republic email: [email protected]
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Abstract

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The Kepler object KOI 2700b was discovered recently as the second exoplanet with a comet-like dusty tail. We aimed at verifying the disintegrating-planet scenario of KOI 2700b by modeling its light curve and to put constraints on various tail and planet properties, as was done in the case of KIC 12557548b. Here, we describe some selected results of our analysis.

Keywords

planets and satellites: generaltechniques: photometricscattering
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S345: Origins: From the Protosun to the First Steps of Life , August 2018 , pp. 244 - 245
Copyright
© International Astronomical Union 2020 

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