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SPITZEROBSERVATIONS OF GJ 3470 b: A VERY LOW-DENSITY NEPTUNE-SIZE PLANET ORBITING A METAL-RICH M DWARF

Demory, Brice-Olivier; Torres, Guillermo; Neves, Vasco; Rogers, Leslie; Gillon, Michaël; Horch, Elliott; Sullivan, Peter; Bonfils, Xavier; Delfosse, Xavier; Forveille, Thierry; Lovis, Christophe; Mayor, Michel; Santos, Nuno; Seager, Sara; Smalley, Barry; Udry, Stephane

Authors

Brice-Olivier Demory

Guillermo Torres

Vasco Neves

Leslie Rogers

Michaël Gillon

Elliott Horch

Peter Sullivan

Xavier Bonfils

Xavier Delfosse

Thierry Forveille

Christophe Lovis

Michel Mayor

Nuno Santos

Sara Seager

Stephane Udry



Abstract

We present Spitzer/IRAC 4.5 μm transit photometry of GJ 3470 b, a Neptune-size planet orbiting an M1.5 dwarf star with a 3.3 day period recently discovered in the course of the HARPS M-dwarf survey. We refine the stellar parameters by employing purely empirical mass–luminosity and surface brightness relations constrained by our updated value for the mean stellar density, and additional information from new near-infrared spectroscopic observations. We derive a stellar mass of $M_{\star } = 0.539^{+0.047}_{-0.043} \,M_{\odot }$ and a radius of $R_{\star } = 0.568^{+0.037}_{-0.031}\,R_{\odot }$. We determine the host star of GJ 3470 b to be metal-rich, with a metallicity of [Fe/H] = +0.20  ±  0.10 and an effective temperature of Teff = 3600  ±  100 K. The revised stellar parameters yield a planetary radius $R_{p} = 4.83_{-0.21}^{+0.22}\,R_{\oplus }$ that is 13% larger than the value previously reported in the literature. We find a planetary mass $M_{p} = 13.9^{+1.5}_{-1.4}\,M_{\oplus }$ that translates to a very low planetary density, $\rho _{p}= 0.72^{+0.13}_{-0.12}$ g cm−3, which is 33% smaller than the original value. With a mean density half of that of GJ 436 b, GJ 3470 b is an example of a very low-density low-mass planet, similar to Kepler-11 d, Kepler-11 e, and Kepler-18 c, but orbiting a much brighter nearby star that is more conducive to follow-up studies.

Citation

Demory, B., Torres, G., Neves, V., Rogers, L., Gillon, M., Horch, E., …Udry, S. SPITZEROBSERVATIONS OF GJ 3470 b: A VERY LOW-DENSITY NEPTUNE-SIZE PLANET ORBITING A METAL-RICH M DWARF. Astrophysical Journal, 768(2), 154. https://doi.org/10.1088/0004-637x/768/2/154

Journal Article Type Article
Online Publication Date Apr 25, 2013
Deposit Date Jun 16, 2023
Journal The Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 768
Issue 2
Pages 154
DOI https://doi.org/10.1088/0004-637x/768/2/154
Keywords Space and Planetary Science; Astronomy and Astrophysics;