IPAC, located on the Caltech campus, is not under direct threat from local fires at this time, though it is subject to the effects of strong winds and poor air quality. Many members of the IPAC community have been impacted by these events, and IPAC will follow Caltech guidance on closures and safe operations. For more information, visit Caltech’s Emergency Updates page at http://www.caltech.edu/emergency.
2mass-planck-allsky

Wolf 503 b: Characterization of a Sub-Neptune Orbiting a Metal-poor K Dwarf

December 2021 • 2021AJ....162..238P

Authors • Polanski, Alex S. • Crossfield, Ian J. M. • Burt, Jennifer A. • Nowak, Grzegorz • López-Morales, Mercedes • Mortier, Annelies • Poretti, Ennio • Behmard, Aida • Benneke, Björn • Blunt, Sarah • Bonomo, Aldo S. • Butler, R. Paul • Chontos, Ashley • Cosentino, Rosario • Crane, Jeffrey D. • Dumusque, Xavier • Fulton, Benjamin J. • Ghedina, Adriano • Gorjian, Varoujan • Grunblatt, Samuel K. • Harutyunyan, Avet • Howard, Andrew W. • Isaacson, Howard • Kosiarek, Molly R. • Latham, David W. • Luque, Rafael • Martinez Fiorenzano, Aldo F. • Mayor, Michel • Mills, Sean M. • Molinari, Emilio • Nagel, Evangelos • Pallé, Enric • Petigura, Erik A. • Shectman, Stephen A. • Sozzetti, Alessandro • Teske, Johanna K. • Wang, Sharon Xuesong • Weiss, Lauren M.

Abstract • Using radial-velocity measurements from four instruments, we report the mass and density of a 2.043 ±0.069 R sub-Neptune orbiting the quiet K-dwarf Wolf 503 (HIP 67285). In addition, we present improved orbital and transit parameters by analyzing previously unused short-cadence K2 campaign 17 photometry and conduct a joint radial-velocity-transit fit to constrain the eccentricity at 0.41 ± 0.05. The addition of a transit observation by Spitzer also allows us to refine the orbital ephemeris in anticipation of further follow-up. Our mass determination, 6.26 ${}_{-0.70}^{+0.69}$ M , in combination with the updated radius measurements, gives Wolf 503 b a bulk density of $\rho ={2.92}_{-0.44}^{+0.50}$ g cm-3. Using interior composition models, we find this density is consistent with an Earth-like core with either a substantial H2O mass fraction (45 ${}_{-16}^{+19}$ %) or a modest H/He envelope (0.5% ± 0.3%). The low H/He mass fraction, along with the old age of Wolf 503 (11 ± 2 Gyr), makes this sub-Neptune an opportune subject for testing theories of XUV-driven mass loss while the brightness of its host (J = 8.3 mag) makes it an attractive target for transmission spectroscopy.

Links


IPAC Authors
(alphabetical)

Bfulton2

Benjamin Fulton

Assistant Scientist