TOI-908: a planet at the edge of the Neptune desert transiting a G-type star

Faith Hawthorn; Daniel Bayliss; David J. Armstrong; Jorge Fernández Fernández; Ares Osborn; Sergio G. Sousa; Vardan Adibekyan; Jeanne Davoult; Karen A. Collins; Yann Alibert; Susana C.C. Barros; François Bouchy; Matteo Brogi; David R. Ciardi; Tansu Daylan; Elisa Delgado Mena; Olivier D.S. Demangeon; Rodrigo F. Díaz; Tianjun Gan; Keith Horne; Sergio Hoyer; Jon M. Jenkins; Eric L.N. Jensen; John F. Kielkopf; Veselin Kostov; David W. Latham; Alan M. Levine; Jorge Lillo-Box; Louise D. Nielsen; Hugh P. Osborn; George R. Ricker; Jose Rodrigues; Nuno C. Santos; Richard P. Schwarz; Sara Seager; Juan Serrano Bell; Avi Shporer; Chris Stockdale; Paul A. Strøm; Peter Tenenbaum; Stephane Udry; Peter J. Wheatley; Joshua N. Winn; Carl Ziegler

doi:10.1093/mnras/stad1840

TOI-908: a planet at the edge of the Neptune desert transiting a G-type star

Faith Hawthorn, Daniel Bayliss, David J. Armstrong, Jorge Fernández Fernández, Ares Osborn, Sergio G. Sousa, Vardan Adibekyan, Jeanne Davoult, Karen A. Collins, Yann Alibert, Susana C.C. Barros, François Bouchy, Matteo Brogi, David R. Ciardi, Tansu Daylan, Elisa Delgado Mena, Olivier D.S. Demangeon, Rodrigo F. Díaz, Tianjun Gan, Keith HorneSergio Hoyer, Jon M. Jenkins, Eric L.N. Jensen, John F. Kielkopf, Veselin Kostov, David W. Latham, Alan M. Levine, Jorge Lillo-Box, Louise D. Nielsen, Hugh P. Osborn, George R. Ricker, Jose Rodrigues, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Juan Serrano Bell, Avi Shporer, Chris Stockdale, Paul A. Strøm, Peter Tenenbaum, Stephane Udry, Peter J. Wheatley, Joshua N. Winn, Carl Ziegler

Physics and Astronomy

Producción científica: Article › revisión exhaustiva

Resumen

An exoplanet, TOI-908 b, orbiting the star TOI-908 (TIC-350153977) has been discovered using TESS data. TOI-908 is a solar-like G-dwarf star with specific mass and radius measurements. The planet, TOI-908 b, has a size of 3.18 R⊕ and orbits its star in 3.18 days. Its mass, determined by HARPS measurements, results in a particular bulk planetary density. Interestingly, TOI-908 b is located in a region known as the Neptune desert, which is sparsely populated by planets. This planet likely originated as a sub-Saturn but has undergone significant photoevaporation due to radiation from its star. As a result, it is expected to continue evaporating, losing a substantial portion of its envelope mass.

Idioma original	English
Páginas (desde-hasta)	3877-3893
Número de páginas	17
Publicación	Monthly Notices of the Royal Astronomical Society
Volumen	524
N.º	3
DOI	https://doi.org/10.1093/mnras/stad1840
Estado	Published - sept 1 2023

ASJC Scopus Subject Areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1093/mnras/stad1840

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Hawthorn, F., Bayliss, D., Armstrong, D. J., Fernández Fernández, J., Osborn, A., Sousa, S. G., Adibekyan, V., Davoult, J., Collins, K. A., Alibert, Y., Barros, S. C. C., Bouchy, F., Brogi, M., Ciardi, D. R., Daylan, T., Delgado Mena, E., Demangeon, O. D. S., Díaz, R. F., Gan, T., ... Ziegler, C. (2023). TOI-908: a planet at the edge of the Neptune desert transiting a G-type star. Monthly Notices of the Royal Astronomical Society, 524(3), 3877-3893. https://doi.org/10.1093/mnras/stad1840

Hawthorn, F, Bayliss, D, Armstrong, DJ, Fernández Fernández, J, Osborn, A, Sousa, SG, Adibekyan, V, Davoult, J, Collins, KA, Alibert, Y, Barros, SCC, Bouchy, F, Brogi, M, Ciardi, DR, Daylan, T, Delgado Mena, E, Demangeon, ODS, Díaz, RF, Gan, T, Horne, K, Hoyer, S, Jenkins, JM, Jensen, ELN, Kielkopf, JF, Kostov, V, Latham, DW, Levine, AM, Lillo-Box, J, Nielsen, LD, Osborn, HP, Ricker, GR, Rodrigues, J, Santos, NC, Schwarz, RP, Seager, S, Serrano Bell, J, Shporer, A, Stockdale, C, Strøm, PA, Tenenbaum, P, Udry, S, Wheatley, PJ, Winn, JN & Ziegler, C 2023, 'TOI-908: a planet at the edge of the Neptune desert transiting a G-type star', Monthly Notices of the Royal Astronomical Society, vol. 524, n.º 3, pp. 3877-3893. https://doi.org/10.1093/mnras/stad1840

@article{3bdb101aa43d4b3087a841fafdadb55a,

title = "TOI-908: a planet at the edge of the Neptune desert transiting a G-type star",

abstract = "An exoplanet, TOI-908 b, orbiting the star TOI-908 (TIC-350153977) has been discovered using TESS data. TOI-908 is a solar-like G-dwarf star with specific mass and radius measurements. The planet, TOI-908 b, has a size of 3.18 R⊕ and orbits its star in 3.18 days. Its mass, determined by HARPS measurements, results in a particular bulk planetary density. Interestingly, TOI-908 b is located in a region known as the Neptune desert, which is sparsely populated by planets. This planet likely originated as a sub-Saturn but has undergone significant photoevaporation due to radiation from its star. As a result, it is expected to continue evaporating, losing a substantial portion of its envelope mass.",

keywords = "planets and satellites: detection, stars: individual: TOI-908 (TIC-350153977, GAIA DR3 46192380870592067842), techniques: photometric, techniques: radial velocities",

author = "Faith Hawthorn and Daniel Bayliss and Armstrong, {David J.} and {Fern{\'a}ndez Fern{\'a}ndez}, Jorge and Ares Osborn and Sousa, {Sergio G.} and Vardan Adibekyan and Jeanne Davoult and Collins, {Karen A.} and Yann Alibert and Barros, {Susana C.C.} and Fran{\c c}ois Bouchy and Matteo Brogi and Ciardi, {David R.} and Tansu Daylan and {Delgado Mena}, Elisa and Demangeon, {Olivier D.S.} and D{\'i}az, {Rodrigo F.} and Tianjun Gan and Keith Horne and Sergio Hoyer and Jenkins, {Jon M.} and Jensen, {Eric L.N.} and Kielkopf, {John F.} and Veselin Kostov and Latham, {David W.} and Levine, {Alan M.} and Jorge Lillo-Box and Nielsen, {Louise D.} and Osborn, {Hugh P.} and Ricker, {George R.} and Jose Rodrigues and Santos, {Nuno C.} and Schwarz, {Richard P.} and Sara Seager and {Serrano Bell}, Juan and Avi Shporer and Chris Stockdale and Str{\o}m, {Paul A.} and Peter Tenenbaum and Stephane Udry and Wheatley, {Peter J.} and Winn, {Joshua N.} and Carl Ziegler",

note = "Funding Information: This paper includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA Explorer Program. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. The TESS team shall assure that the masses of fifty (50) planets with radii less than 4 REarth are determined. Funding Information: This work makes use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Funding Information: This work makes use of observations from the LCOGT network. Part of the LCOGT telescope time was granted by NOIRLab through the Mid-Scale Innovations Program (MSIP). MSIP is funded by NSF. Publisher Copyright: {\textcopyright} 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2023",

month = sep,

day = "1",

doi = "10.1093/mnras/stad1840",

language = "English",

volume = "524",

pages = "3877--3893",

number = "3",

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TY - JOUR

T1 - TOI-908

T2 - a planet at the edge of the Neptune desert transiting a G-type star

AU - Hawthorn, Faith

AU - Bayliss, Daniel

AU - Armstrong, David J.

AU - Fernández Fernández, Jorge

AU - Osborn, Ares

AU - Sousa, Sergio G.

AU - Adibekyan, Vardan

AU - Davoult, Jeanne

AU - Collins, Karen A.

AU - Alibert, Yann

AU - Barros, Susana C.C.

AU - Bouchy, François

AU - Brogi, Matteo

AU - Ciardi, David R.

AU - Daylan, Tansu

AU - Delgado Mena, Elisa

AU - Demangeon, Olivier D.S.

AU - Díaz, Rodrigo F.

AU - Gan, Tianjun

AU - Horne, Keith

AU - Hoyer, Sergio

AU - Jenkins, Jon M.

AU - Jensen, Eric L.N.

AU - Kielkopf, John F.

AU - Kostov, Veselin

AU - Latham, David W.

AU - Levine, Alan M.

AU - Lillo-Box, Jorge

AU - Nielsen, Louise D.

AU - Osborn, Hugh P.

AU - Ricker, George R.

AU - Rodrigues, Jose

AU - Santos, Nuno C.

AU - Schwarz, Richard P.

AU - Seager, Sara

AU - Serrano Bell, Juan

AU - Shporer, Avi

AU - Stockdale, Chris

AU - Strøm, Paul A.

AU - Tenenbaum, Peter

AU - Udry, Stephane

AU - Wheatley, Peter J.

AU - Winn, Joshua N.

AU - Ziegler, Carl

N1 - Funding Information: This paper includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA Explorer Program. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. The TESS team shall assure that the masses of fifty (50) planets with radii less than 4 REarth are determined. Funding Information: This work makes use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Funding Information: This work makes use of observations from the LCOGT network. Part of the LCOGT telescope time was granted by NOIRLab through the Mid-Scale Innovations Program (MSIP). MSIP is funded by NSF. Publisher Copyright: © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

PY - 2023/9/1

Y1 - 2023/9/1

N2 - An exoplanet, TOI-908 b, orbiting the star TOI-908 (TIC-350153977) has been discovered using TESS data. TOI-908 is a solar-like G-dwarf star with specific mass and radius measurements. The planet, TOI-908 b, has a size of 3.18 R⊕ and orbits its star in 3.18 days. Its mass, determined by HARPS measurements, results in a particular bulk planetary density. Interestingly, TOI-908 b is located in a region known as the Neptune desert, which is sparsely populated by planets. This planet likely originated as a sub-Saturn but has undergone significant photoevaporation due to radiation from its star. As a result, it is expected to continue evaporating, losing a substantial portion of its envelope mass.

AB - An exoplanet, TOI-908 b, orbiting the star TOI-908 (TIC-350153977) has been discovered using TESS data. TOI-908 is a solar-like G-dwarf star with specific mass and radius measurements. The planet, TOI-908 b, has a size of 3.18 R⊕ and orbits its star in 3.18 days. Its mass, determined by HARPS measurements, results in a particular bulk planetary density. Interestingly, TOI-908 b is located in a region known as the Neptune desert, which is sparsely populated by planets. This planet likely originated as a sub-Saturn but has undergone significant photoevaporation due to radiation from its star. As a result, it is expected to continue evaporating, losing a substantial portion of its envelope mass.

KW - planets and satellites: detection

KW - stars: individual: TOI-908 (TIC-350153977, GAIA DR3 46192380870592067842)

KW - techniques: photometric

KW - techniques: radial velocities

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