A New Analysis of the Exoplanet Hosting System HD 6434
Natalie R. Hinkel; Stephen R. Kane; Genady Pilyavsky; Tabetha S. Boyajian; David J. James; Dominique Naef; Debra A. Fischer; Stephane Udry · 2015 · arXiv
WASTE classifies this as Negative / Null Result Report · AI classification, approximate
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Abstract (excerpt)
The current goal of exoplanetary science is not only focused on detecting but characterizing planetary systems in hopes of understanding how they formed, evolved, and relate to the Solar System. The Transit Ephemeris Refinement and Monitoring Survey (TERMS) combines both radial velocity (RV) and photometric data in order to achieve unprecedented ground-based precision in the fundamental properties of nearby, bright, exoplanet-hosting systems. Here we discuss HD 6434 and its planet, HD 6434b, which has a M_p*sin(i) = 0.44 M_J mass and orbits every 22.0170 days with an eccentricity of 0.146. We
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Metadata source: arXiv