H P Osborn
Two warm Neptunes transiting HIP 9618 revealed by <i>TESS</i> and <i>Cheops</i>
Osborn, H P; Nowak, G; Hébrard, G; Masseron, T; Lillo-Box, J; Pallé, E; Bekkelien, A; Florén, H-G; Guterman, P; Simon, A E; Adibekyan, V; Bieryla, A; Borsato, L; Brandeker, A; Ciardi, D R; Collier Cameron, A; Collins, K A; Egger, J A; Gandolfi, D; Hooton, M J; Latham, D W; Lendl, M; Matthews, E C; Tuson, A; Ulmer-Moll, S; Vanderburg, A; Wilson, T G; Ziegler, C; Alibert, Y; Alonso, R; Anglada, G; Arnold, L; Asquier, J; Barrado y Navascues, D; Baumjohann, W; Beck, T; Belinski, A A; Benz, W; Biondi, F; Boisse, I; Bonfils, X; Broeg, C; Buchhave, L A; Bárczy, T; Barros, S C C; Cabrera, J; Cardona Guillen, C; Carleo, I; Castro-González, A; Charnoz, S; Christiansen, J; Cortes-Zuleta, P; Csizmadia, S; Dalal, S; Davies, M B; Deleuil, M; Delfosse, X; Delrez, L; Demory, B-O; Dunlavey, A B; Ehrenreich, D; Erikson, A; Fernandes, R B; Fortier, A; Forveille, T; Fossati, L; Fridlund, M; Gillon, M; Goeke, R F; Goliguzova, M V; Gonzales, E J; Günther, M N; Güdel, M; Heidari, N; Henze, C E; Howell, S; Ho...
Authors
G Nowak
G Hébrard
T Masseron
J Lillo-Box
E Pallé
A Bekkelien
H-G Florén
P Guterman
A E Simon
V Adibekyan
A Bieryla
L Borsato
A Brandeker
D R Ciardi
A Collier Cameron
K A Collins
J A Egger
D Gandolfi
M J Hooton
D W Latham
M Lendl
E C Matthews
A Tuson
S Ulmer-Moll
A Vanderburg
T G Wilson
C Ziegler
Y Alibert
R Alonso
G Anglada
L Arnold
J Asquier
D Barrado y Navascues
W Baumjohann
T Beck
A A Belinski
W Benz
F Biondi
I Boisse
X Bonfils
C Broeg
L A Buchhave
T Bárczy
S C C Barros
J Cabrera
C Cardona Guillen
I Carleo
A Castro-González
S Charnoz
J Christiansen
P Cortes-Zuleta
S Csizmadia
S Dalal
M B Davies
M Deleuil
X Delfosse
L Delrez
B-O Demory
A B Dunlavey
D Ehrenreich
A Erikson
R B Fernandes
A Fortier
T Forveille
L Fossati
M Fridlund
M Gillon
R F Goeke
M V Goliguzova
E J Gonzales
M N Günther
M Güdel
N Heidari
C E Henze
S Howell
S Hoyer
J I Frey
K G Isaak
J M Jenkins
F Kiefer
L Kiss
J Korth
Pierre Maxted p.maxted@keele.ac.uk
J Laskar
A Lecavelier des Etangs
C Lovis
M B Lund
R Luque
D Magrin
J M Almenara
E Martioli
M Mecina
J V Medina
D Moldovan
M Morales-Calderón
G Morello
C Moutou
F Murgas
E L N Jensen
V Nascimbeni
G Olofsson
R Ottensamer
I Pagano
G Peter
G Piotto
D Pollacco
D Queloz
R Ragazzoni
N Rando
H Rauer
I Ribas
G Ricker
O D S Demangeon
A M S Smith
N Santos
G Scandariato
S Seager
S G Sousa
M Steller
G M Szabó
D Ségransan
N Thomas
S Udry
B Ulmer
V Van Grootel
R Vanderspek
N Walton
J N Winn
Abstract
HIP 9618 (HD 12572, TOI-1471, TIC 306263608) is a bright (G = 9.0 mag) solar analogue. TESS photometry revealed the star to have two candidate planets with radii of 3.9 ± 0.044 R⊕ (HIP 9618 b) and 3.343 ± 0.039 R⊕ (HIP 9618 c). While the 20.77291 d period of HIP 9618 b was measured unambiguously, HIP 9618 c showed only two transits separated by a 680-d gap in the time series, leaving many possibilities for the period. To solve this issue, CHEOPS performed targeted photometry of period aliases to attempt to recover the true period of planet c, and successfully determined the true period to be 52.56349 d. High-resolution spectroscopy with HARPS-N, SOPHIE, and CAFE revealed a mass of 10.0 ± 3.1M⊕ for HIP 9618 b, which, according to our interior structure models, corresponds to a $6.8\pm 1.4~{{\ \rm per\ cent}}$ gas fraction. HIP 9618 c appears to have a lower mass than HIP 9618 b, with a 3-sigma upper limit of &lt;18M⊕. Follow-up and archival RV measurements also reveal a clear long-term trend which, when combined with imaging and astrometric information, reveal a low-mass companion ($0.08^{+0.12}_{-0.05} M_\odot$) orbiting at $26.0^{+19.0}_{-11.0}$ au. This detection makes HIP 9618 one of only five bright (K &lt; 8 mag) transiting multiplanet systems known to host a planet with P &gt; 50 d, opening the door for the atmospheric characterization of warm (Teq &lt; 750 K) sub-Neptunes.
Citation
Osborn, H. P., Nowak, G., Hébrard, G., Masseron, T., Lillo-Box, J., Pallé, E., …Winn, J. N. (2023). Two warm Neptunes transiting HIP 9618 revealed by TESS and Cheops. Monthly Notices of the Royal Astronomical Society, 523(2), 3069-3089. https://doi.org/10.1093/mnras/stad1319
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 5, 2023 |
Online Publication Date | Jun 8, 2023 |
Publication Date | May 30, 2023 |
Deposit Date | Jun 29, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 523 |
Issue | 2 |
Pages | 3069-3089 |
DOI | https://doi.org/10.1093/mnras/stad1319 |
Keywords | Space and Planetary Science, Astronomy and Astrophysics |
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