X-ray emission from the super-Earth host GJ 1214

Abstract

Stellar activity can produce large amounts of high-energy radiation, which is absorbed by the planetary atmosphere leading to irradiation-driven mass loss. We present the detection and an investigation of high-energy emission in a transiting super-Earth host system, GJ 1214, based on XMM-Newton observations. We derive an X-ray luminosity of LX = 7.4 × 1025 erg s -1 and a corresponding activity level of log (LX /L bol) -5.3. Further, we determine a coronal temperature of about 3.5 MK, which is typical for coronal emission of moderately active low-mass stars. We estimate that GJ 1214 b evaporates at a rate of 1.3× 1010 g s-1 and has lost a total of 2-5.6 M ⊕. © 2014. The American Astronomical Society. All rights reserved..