TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned

Jack Lubin; Xian Yu Wang; Malena Rice; Jiayin Dong; Songhu Wang; Brandon T. Radzom; Paul Robertson; Gudmundur Stefansson; Jaime A. Alvarado-Montes; Corey Beard; Chad F. Bender; Arvind F. Gupta; Samuel Halverson; Shubham Kanodia; Dan Li; Andrea S.J. Lin; Sarah E. Logsdon; Emily Lubar; Suvrath Mahadevan; Joe P. Ninan; Jayadev Rajagopal; Arpita Roy; Christian Schwab; Jason T. Wright

doi:10.3847/2041-8213/ad0fea

TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned

Jack Lubin
, Xian Yu Wang
, Malena Rice
, Jiayin Dong
, Songhu Wang
, Brandon T. Radzom
, Paul Robertson
, Gudmundur Stefansson
, Jaime A. Alvarado-Montes
, Corey Beard
, Chad F. Bender
, Arvind F. Gupta
, Samuel Halverson
, Shubham Kanodia
, Dan Li
, Andrea S.J. Lin
, Sarah E. Logsdon
, Emily Lubar
, Suvrath Mahadevan
, Joe P. Ninan

Jayadev Rajagopal, Arpita Roy, Christian Schwab, Jason T. Wright

Steward Observatory

Research output: Contribution to journal › Article › peer-review

9 Scopus citations

Abstract

We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter-McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN Telescope at Kitt Peak National Observatory. TOI-1670 hosts a sub-Neptune (P ∼ 11 days; planet b) interior to the warm Jovian (P ∼ 40 days; planet c), which presents an opportunity to investigate the dynamics of a warm Jupiter with an inner companion. Additionally, TOI-1670 c is now among the longest-period planets to date to have its sky-projected obliquity angle measured. We find planet c is well aligned to the host star, with λ = − 0.°3 ± 2.°2. TOI-1670 c joins a growing census of aligned warm Jupiters around single stars and aligned planets in multiplanet systems.

Original language	English (US)
Article number	L5
Journal	Astrophysical Journal Letters
Volume	959
Issue number	1
DOIs	https://doi.org/10.3847/2041-8213/ad0fea
State	Published - Dec 1 2023

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.3847/2041-8213/ad0fea

Cite this

Lubin, J., Wang, X. Y., Rice, M., Dong, J., Wang, S., Radzom, B. T., Robertson, P., Stefansson, G., Alvarado-Montes, J. A., Beard, C., Bender, C. F., Gupta, A. F., Halverson, S., Kanodia, S., Li, D., Lin, A. S. J., Logsdon, S. E., Lubar, E., Mahadevan, S., ... Wright, J. T. (2023). TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned. Astrophysical Journal Letters, 959(1), Article L5. https://doi.org/10.3847/2041-8213/ad0fea

Lubin, J, Wang, XY, Rice, M, Dong, J, Wang, S, Radzom, BT, Robertson, P, Stefansson, G, Alvarado-Montes, JA, Beard, C, Bender, CF, Gupta, AF, Halverson, S, Kanodia, S, Li, D, Lin, ASJ, Logsdon, SE, Lubar, E, Mahadevan, S, Ninan, JP, Rajagopal, J, Roy, A, Schwab, C & Wright, JT 2023, 'TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned', Astrophysical Journal Letters, vol. 959, no. 1, L5. https://doi.org/10.3847/2041-8213/ad0fea

@article{6908ac0ad1004e58a95e0e825ce47292,

title = "TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned",

abstract = "We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter-McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN Telescope at Kitt Peak National Observatory. TOI-1670 hosts a sub-Neptune (P ∼ 11 days; planet b) interior to the warm Jovian (P ∼ 40 days; planet c), which presents an opportunity to investigate the dynamics of a warm Jupiter with an inner companion. Additionally, TOI-1670 c is now among the longest-period planets to date to have its sky-projected obliquity angle measured. We find planet c is well aligned to the host star, with λ = − 0.°3 ± 2.°2. TOI-1670 c joins a growing census of aligned warm Jupiters around single stars and aligned planets in multiplanet systems.",

author = "Jack Lubin and Wang, \{Xian Yu\} and Malena Rice and Jiayin Dong and Songhu Wang and Radzom, \{Brandon T.\} and Paul Robertson and Gudmundur Stefansson and Alvarado-Montes, \{Jaime A.\} and Corey Beard and Bender, \{Chad F.\} and Gupta, \{Arvind F.\} and Samuel Halverson and Shubham Kanodia and Dan Li and Lin, \{Andrea S.J.\} and Logsdon, \{Sarah E.\} and Emily Lubar and Suvrath Mahadevan and Ninan, \{Joe P.\} and Jayadev Rajagopal and Arpita Roy and Christian Schwab and Wright, \{Jason T.\}",

note = "Publisher Copyright: {\textcopyright} 2023. The Author(s). Published by the American Astronomical Society.",

year = "2023",

month = dec,

day = "1",

doi = "10.3847/2041-8213/ad0fea",

language = "English (US)",

volume = "959",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

number = "1",

}

TY - JOUR

T1 - TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned

AU - Lubin, Jack

AU - Wang, Xian Yu

AU - Rice, Malena

AU - Dong, Jiayin

AU - Wang, Songhu

AU - Radzom, Brandon T.

AU - Robertson, Paul

AU - Stefansson, Gudmundur

AU - Alvarado-Montes, Jaime A.

AU - Beard, Corey

AU - Bender, Chad F.

AU - Gupta, Arvind F.

AU - Halverson, Samuel

AU - Kanodia, Shubham

AU - Li, Dan

AU - Lin, Andrea S.J.

AU - Logsdon, Sarah E.

AU - Lubar, Emily

AU - Mahadevan, Suvrath

AU - Ninan, Joe P.

AU - Rajagopal, Jayadev

AU - Roy, Arpita

AU - Schwab, Christian

AU - Wright, Jason T.

PY - 2023/12/1

Y1 - 2023/12/1

N2 - We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter-McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN Telescope at Kitt Peak National Observatory. TOI-1670 hosts a sub-Neptune (P ∼ 11 days; planet b) interior to the warm Jovian (P ∼ 40 days; planet c), which presents an opportunity to investigate the dynamics of a warm Jupiter with an inner companion. Additionally, TOI-1670 c is now among the longest-period planets to date to have its sky-projected obliquity angle measured. We find planet c is well aligned to the host star, with λ = − 0.°3 ± 2.°2. TOI-1670 c joins a growing census of aligned warm Jupiters around single stars and aligned planets in multiplanet systems.

AB - We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter-McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN Telescope at Kitt Peak National Observatory. TOI-1670 hosts a sub-Neptune (P ∼ 11 days; planet b) interior to the warm Jovian (P ∼ 40 days; planet c), which presents an opportunity to investigate the dynamics of a warm Jupiter with an inner companion. Additionally, TOI-1670 c is now among the longest-period planets to date to have its sky-projected obliquity angle measured. We find planet c is well aligned to the host star, with λ = − 0.°3 ± 2.°2. TOI-1670 c joins a growing census of aligned warm Jupiters around single stars and aligned planets in multiplanet systems.

UR - https://www.scopus.com/pages/publications/85180094833

UR - https://www.scopus.com/pages/publications/85180094833#tab=citedBy

U2 - 10.3847/2041-8213/ad0fea

DO - 10.3847/2041-8213/ad0fea

M3 - Article

AN - SCOPUS:85180094833

SN - 2041-8205

VL - 959

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 1

M1 - L5

ER -

TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this