TY - JOUR
T1 - Evidence for He I 10830 Å absorption during the transit of a warm Neptune around the M-dwarf GJ 3470 with the Habitable-zone Planet Finder
AU - Ninan, Joe P.
AU - Stefansson, Gudmundur
AU - Mahadevan, Suvrath
AU - Bender, Chad
AU - Robertson, Paul
AU - Ramsey, Lawrence
AU - Terrien, Ryan
AU - Wright, Jason
AU - Diddams, Scott A.
AU - Kanodia, Shubham
AU - Cochran, William
AU - Endl, Michael
AU - Ford, Eric B.
AU - Fredrick, Connor
AU - Halverson, Samuel
AU - Hearty, Fred
AU - Jennings, Jeff
AU - Kaplan, Kyle
AU - Lubar, Emily
AU - Metcalf, Andrew J.
AU - Monson, Andrew
AU - Nitroy, Colin
AU - Roy, Arpita
AU - Schwab, Christian
PY - 2020/5/10
Y1 - 2020/5/10
N2 - Understanding the dynamics and kinematics of outflowing atmospheres of hot and warm exoplanets is crucial to understanding the origins and evolutionary history of the exoplanets near the evaporation desert. Recently, ground-based measurements of the meta-stable helium atom's resonant absorption at 10830 Å has become a powerful probe of the base environment which is driving the outflow of exoplanet atmospheres. We report evidence for the He i 10830 Å in absorption (equivalent width ∼0.012 ± 0.002 Å) in the exosphere of a warm Neptune orbiting the M-dwarf GJ 3470, during three transits using the Habitable Zone Planet Finder near-infrared spectrograph. This marks the first reported evidence for He I 10830 Å atmospheric absorption for a planet orbiting an M-dwarf. Our detected absorption is broad and its blueshifted wing extends to-36 km s-1, the largest reported in the literature to date. We modeled the state of helium atoms in the exosphere of GJ3470b based on assumptions on the UV and X-ray flux of GJ 3470, and found our measurement of flux-weighted column density of meta-stable state helium (NHe 23S = 2.4 x 1010 cm-2), derived from our transit observations, to be consistent with the model, within its uncertainties. The methodology developed here will be useful to study and constrain the atmospheric outflow models of other exoplanets like GJ 3470b, which are near the edge of the evaporation desert.
AB - Understanding the dynamics and kinematics of outflowing atmospheres of hot and warm exoplanets is crucial to understanding the origins and evolutionary history of the exoplanets near the evaporation desert. Recently, ground-based measurements of the meta-stable helium atom's resonant absorption at 10830 Å has become a powerful probe of the base environment which is driving the outflow of exoplanet atmospheres. We report evidence for the He i 10830 Å in absorption (equivalent width ∼0.012 ± 0.002 Å) in the exosphere of a warm Neptune orbiting the M-dwarf GJ 3470, during three transits using the Habitable Zone Planet Finder near-infrared spectrograph. This marks the first reported evidence for He I 10830 Å atmospheric absorption for a planet orbiting an M-dwarf. Our detected absorption is broad and its blueshifted wing extends to-36 km s-1, the largest reported in the literature to date. We modeled the state of helium atoms in the exosphere of GJ3470b based on assumptions on the UV and X-ray flux of GJ 3470, and found our measurement of flux-weighted column density of meta-stable state helium (NHe 23S = 2.4 x 1010 cm-2), derived from our transit observations, to be consistent with the model, within its uncertainties. The methodology developed here will be useful to study and constrain the atmospheric outflow models of other exoplanets like GJ 3470b, which are near the edge of the evaporation desert.
UR - http://www.scopus.com/inward/record.url?scp=85085320216&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ab8559
DO - 10.3847/1538-4357/ab8559
M3 - Article
VL - 894
SP - 1
EP - 9
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 97
ER -