An ablating super-Earth in an eccentric binary from the Dispersed Matter Planet Project
Abstract
Earth mass exoplanets are difficult to detect. The Dispersed Matter Planet Project (DMPP) identifies stars which are likely to host the most detectable low mass exoplanets. The star DMPP-3 (HD 42936) shows signs of circumstellar absorption, indicative of mass loss from ablating planets. Here we report the radial velocity (RV) discovery of a highly eccentric 507 d binary companion and a hot super-Earth planet in a 6.67 d orbit around the primary star. DMPP-3A is a solar type star while DMPP-3B is just massive enough to fuse hydrogen. The binary, with semi-major axis 1.22 0.02 AU, is considerably tighter than others known to host planets orbiting only one of the component stars. The configuration of the DMPP-3 planetary system is rare and indicates dynamical interactions, though the evolutionary history is not entirely clear. DMPP-3Ab is possibly the residual core of a giant planet precursor, consistent with the inferred circumstellar gas shroud.
Cite
@article{arxiv.1912.10793,
title = {An ablating super-Earth in an eccentric binary from the Dispersed Matter Planet Project},
author = {John R. Barnes and Carole A. Haswell and Daniel Staab and Guillem Anglada-Escudé and Luca Fossati and James P. J. Doherty and Joseph Cooper and James S. Jenkins and Matías R. Díaz and Maritza G. Soto and Pablo A. Peña Rojas},
journal= {arXiv preprint arXiv:1912.10793},
year = {2019}
}
Comments
Accepted for publication by Nature Astronomy on 12th November 2019 (Main article, Methods and Supplementary Information; 18 pages, 4 figures, 3 tables)