An ultrahot Neptune in the Neptune desert

James S. Jenkins; Matías R. Díaz; Nicolás T. Kurtovic; Néstor Espinoza; Jose I. Vines; Pablo A.Peña Rojas; Rafael Brahm; Pascal Torres; Pía Cortés-Zuleta; Maritza G. Soto; Eric D. Lopez; George W. King; Peter J. Wheatley; Joshua N. Winn; David R. Ciardi; George Ricker; Roland Vanderspek; David W. Latham; Sara Seager; Jon M. Jenkins; Charles A. Beichman; Allyson Bieryla; Christopher J. Burke; Jessie L. Christiansen; Christopher E. Henze; Todd C. Klaus; Sean McCauliff; Mayuko Mori; Norio Narita; Taku Nishiumi; Motohide Tamura; Jerome Pitogo de Leon; Samuel N. Quinn; Jesus Noel Villaseñor; Michael Vezie; Jack J. Lissauer; Karen A. Collins; Kevin I. Collins; Giovanni Isopi; Franco Mallia; Andrea Ercolino; Cristobal Petrovich; Andrés Jordán; Jack S. Acton; David J. Armstrong; Daniel Bayliss; François Bouchy; Claudia Belardi; Edward M. Bryant; Matthew R. Burleigh; Juan Cabrera; Sarah L. Casewell; Alexander Chaushev; Benjamin F. Cooke; Philipp Eigmüller; Anders Erikson; Emma Foxell; Boris T. Gänsicke; Samuel Gill; Edward Gillen; Maximilian N. Günther; Michael R. Goad; Matthew J. Hooton; James A.G. Jackman; Tom Louden; James McCormac; Maximiliano Moyano; Louise D. Nielsen; Don Pollacco; Didier Queloz; Heike Rauer; Liam Raynard; Alexis M.S. Smith; Rosanna H. Tilbrook; Ruth Titz-Weider; Oliver Turner; Stéphane Udry; Simon R. Walker; Christopher A. Watson; Richard G. West; Enric Palle; Carl Ziegler; Nicholas Law; Andrew W. Mann

doi:10.1038/s41550-020-1142-z

An ultrahot Neptune in the Neptune desert

James S. Jenkins, Matías R. Díaz, Nicolás T. Kurtovic, Néstor Espinoza, Jose I. Vines, Pablo A.Peña Rojas, Rafael Brahm, Pascal Torres, Pía Cortés-Zuleta, Maritza G. Soto, Eric D. Lopez, George W. King, Peter J. Wheatley, Joshua N. Winn, David R. Ciardi, George Ricker, Roland Vanderspek, David W. Latham, Sara Seager, Jon M. JenkinsCharles A. Beichman, Allyson Bieryla, Christopher J. Burke, Jessie L. Christiansen, Christopher E. Henze, Todd C. Klaus, Sean McCauliff, Mayuko Mori, Norio Narita, Taku Nishiumi, Motohide Tamura, Jerome Pitogo de Leon, Samuel N. Quinn, Jesus Noel Villaseñor, Michael Vezie, Jack J. Lissauer, Karen A. Collins, Kevin I. Collins, Giovanni Isopi, Franco Mallia, Andrea Ercolino, Cristobal Petrovich, Andrés Jordán, Jack S. Acton, David J. Armstrong, Daniel Bayliss, François Bouchy, Claudia Belardi, Edward M. Bryant, Matthew R. Burleigh, Juan Cabrera, Sarah L. Casewell, Alexander Chaushev, Benjamin F. Cooke, Philipp Eigmüller, Anders Erikson, Emma Foxell, Boris T. Gänsicke, Samuel Gill, Edward Gillen, Maximilian N. Günther, Michael R. Goad, Matthew J. Hooton, James A.G. Jackman, Tom Louden, James McCormac, Maximiliano Moyano, Louise D. Nielsen, Don Pollacco, Didier Queloz, Heike Rauer, Liam Raynard, Alexis M.S. Smith, Rosanna H. Tilbrook, Ruth Titz-Weider, Oliver Turner, Stéphane Udry, Simon R. Walker, Christopher A. Watson, Richard G. West, Enric Palle, Carl Ziegler, Nicholas Law, Andrew W. Mann

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Resumen

About 1 out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultrashort-period planet^1,2. All of the previously known ultrashort-period planets are either hot Jupiters, with sizes above 10 Earth radii (R_⊕), or apparently rocky planets smaller than 2 R_⊕. Such lack of planets of intermediate size (the ‘hot Neptune desert’) has been interpreted as the inability of low-mass planets to retain any hydrogen/helium (H/He) envelope in the face of strong stellar irradiation. Here we report the discovery of an ultrashort-period planet with a radius of 4.6 R_⊕ and a mass of 29 M_⊕, firmly in the hot Neptune desert. Data from the Transiting Exoplanet Survey Satellite³ revealed transits of the bright Sun-like star LTT 9779 every 0.79 days. The planet’s mean density is similar to that of Neptune, and according to thermal evolution models, it has a H/He-rich envelope constituting 9.0−2.9+2.7% of the total mass. With an equilibrium temperature around 2,000 K, it is unclear how this ‘ultrahot Neptune’ managed to retain such an envelope. Follow-up observations of the planet’s atmosphere to better understand its origin and physical nature will be facilitated by the star’s brightness (V_mag = 9.8).

Idioma original	Inglés
Páginas (desde-hasta)	1148-1157
Número de páginas	10
Publicación	Nature Astronomy
Volumen	4
N.º	12
DOI	https://doi.org/10.1038/s41550-020-1142-z
Estado	Publicada - dic. 2020
Publicado de forma externa	Sí

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Jenkins, J. S., Díaz, M. R., Kurtovic, N. T., Espinoza, N., Vines, J. I., Rojas, P. A. P., Brahm, R., Torres, P., Cortés-Zuleta, P., Soto, M. G., Lopez, E. D., King, G. W., Wheatley, P. J., Winn, J. N., Ciardi, D. R., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., ... Mann, A. W. (2020). An ultrahot Neptune in the Neptune desert. Nature Astronomy, 4(12), 1148-1157. https://doi.org/10.1038/s41550-020-1142-z

@article{c3febd2748fe4d15b953d0a6c58c7fcb,

title = "An ultrahot Neptune in the Neptune desert",

abstract = "About 1 out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultrashort-period planet1,2. All of the previously known ultrashort-period planets are either hot Jupiters, with sizes above 10 Earth radii (R⊕), or apparently rocky planets smaller than 2 R⊕. Such lack of planets of intermediate size (the {\textquoteleft}hot Neptune desert{\textquoteright}) has been interpreted as the inability of low-mass planets to retain any hydrogen/helium (H/He) envelope in the face of strong stellar irradiation. Here we report the discovery of an ultrashort-period planet with a radius of 4.6 R⊕ and a mass of 29 M⊕, firmly in the hot Neptune desert. Data from the Transiting Exoplanet Survey Satellite3 revealed transits of the bright Sun-like star LTT 9779 every 0.79 days. The planet{\textquoteright}s mean density is similar to that of Neptune, and according to thermal evolution models, it has a H/He-rich envelope constituting 9.0−2.9+2.7% of the total mass. With an equilibrium temperature around 2,000 K, it is unclear how this {\textquoteleft}ultrahot Neptune{\textquoteright} managed to retain such an envelope. Follow-up observations of the planet{\textquoteright}s atmosphere to better understand its origin and physical nature will be facilitated by the star{\textquoteright}s brightness (Vmag = 9.8).",

author = "Jenkins, {James S.} and D{\'i}az, {Mat{\'i}as R.} and Kurtovic, {Nicol{\'a}s T.} and N{\'e}stor Espinoza and Vines, {Jose I.} and Rojas, {Pablo A.Pe{\~n}a} and Rafael Brahm and Pascal Torres and P{\'i}a Cort{\'e}s-Zuleta and Soto, {Maritza G.} and Lopez, {Eric D.} and King, {George W.} and Wheatley, {Peter J.} and Winn, {Joshua N.} and Ciardi, {David R.} and George Ricker and Roland Vanderspek and Latham, {David W.} and Sara Seager and Jenkins, {Jon M.} and Beichman, {Charles A.} and Allyson Bieryla and Burke, {Christopher J.} and Christiansen, {Jessie L.} and Henze, {Christopher E.} and Klaus, {Todd C.} and Sean McCauliff and Mayuko Mori and Norio Narita and Taku Nishiumi and Motohide Tamura and {de Leon}, {Jerome Pitogo} and Quinn, {Samuel N.} and Villase{\~n}or, {Jesus Noel} and Michael Vezie and Lissauer, {Jack J.} and Collins, {Karen A.} and Collins, {Kevin I.} and Giovanni Isopi and Franco Mallia and Andrea Ercolino and Cristobal Petrovich and Andr{\'e}s Jord{\'a}n and Acton, {Jack S.} and Armstrong, {David J.} and Daniel Bayliss and Fran{\c c}ois Bouchy and Claudia Belardi and Bryant, {Edward M.} and Burleigh, {Matthew R.} and Juan Cabrera and Casewell, {Sarah L.} and Alexander Chaushev and Cooke, {Benjamin F.} and Philipp Eigm{\"u}ller and Anders Erikson and Emma Foxell and G{\"a}nsicke, {Boris T.} and Samuel Gill and Edward Gillen and G{\"u}nther, {Maximilian N.} and Goad, {Michael R.} and Hooton, {Matthew J.} and Jackman, {James A.G.} and Tom Louden and James McCormac and Maximiliano Moyano and Nielsen, {Louise D.} and Don Pollacco and Didier Queloz and Heike Rauer and Liam Raynard and Smith, {Alexis M.S.} and Tilbrook, {Rosanna H.} and Ruth Titz-Weider and Oliver Turner and St{\'e}phane Udry and Walker, {Simon R.} and Watson, {Christopher A.} and West, {Richard G.} and Enric Palle and Carl Ziegler and Nicholas Law and Mann, {Andrew W.}",

note = "Publisher Copyright: {\textcopyright} 2020, The Author(s), under exclusive licence to Springer Nature Limited.",

year = "2020",

month = dec,

doi = "10.1038/s41550-020-1142-z",

language = "English",

volume = "4",

pages = "1148--1157",

journal = "Nature Astronomy",

issn = "2397-3366",

publisher = "Nature Publishing Group",

number = "12",

}

Jenkins, JS, Díaz, MR, Kurtovic, NT, Espinoza, N, Vines, JI, Rojas, PAP, Brahm, R, Torres, P, Cortés-Zuleta, P, Soto, MG, Lopez, ED, King, GW, Wheatley, PJ, Winn, JN, Ciardi, DR, Ricker, G, Vanderspek, R, Latham, DW, Seager, S, Jenkins, JM, Beichman, CA, Bieryla, A, Burke, CJ, Christiansen, JL, Henze, CE, Klaus, TC, McCauliff, S, Mori, M, Narita, N, Nishiumi, T, Tamura, M, de Leon, JP, Quinn, SN, Villaseñor, JN, Vezie, M, Lissauer, JJ, Collins, KA, Collins, KI, Isopi, G, Mallia, F, Ercolino, A, Petrovich, C, Jordán, A, Acton, JS, Armstrong, DJ, Bayliss, D, Bouchy, F, Belardi, C, Bryant, EM, Burleigh, MR, Cabrera, J, Casewell, SL, Chaushev, A, Cooke, BF, Eigmüller, P, Erikson, A, Foxell, E, Gänsicke, BT, Gill, S, Gillen, E, Günther, MN, Goad, MR, Hooton, MJ, Jackman, JAG, Louden, T, McCormac, J, Moyano, M, Nielsen, LD, Pollacco, D, Queloz, D, Rauer, H, Raynard, L, Smith, AMS, Tilbrook, RH, Titz-Weider, R, Turner, O, Udry, S, Walker, SR, Watson, CA, West, RG, Palle, E, Ziegler, C, Law, N & Mann, AW 2020, 'An ultrahot Neptune in the Neptune desert', Nature Astronomy, vol. 4, n.º 12, pp. 1148-1157. https://doi.org/10.1038/s41550-020-1142-z

TY - JOUR

T1 - An ultrahot Neptune in the Neptune desert

AU - Jenkins, James S.

AU - Díaz, Matías R.

AU - Kurtovic, Nicolás T.

AU - Espinoza, Néstor

AU - Vines, Jose I.

AU - Rojas, Pablo A.Peña

AU - Brahm, Rafael

AU - Torres, Pascal

AU - Cortés-Zuleta, Pía

AU - Soto, Maritza G.

AU - Lopez, Eric D.

AU - King, George W.

AU - Wheatley, Peter J.

AU - Winn, Joshua N.

AU - Ciardi, David R.

AU - Ricker, George

AU - Vanderspek, Roland

AU - Latham, David W.

AU - Seager, Sara

AU - Jenkins, Jon M.

AU - Beichman, Charles A.

AU - Bieryla, Allyson

AU - Burke, Christopher J.

AU - Christiansen, Jessie L.

AU - Henze, Christopher E.

AU - Klaus, Todd C.

AU - McCauliff, Sean

AU - Mori, Mayuko

AU - Narita, Norio

AU - Nishiumi, Taku

AU - Tamura, Motohide

AU - de Leon, Jerome Pitogo

AU - Quinn, Samuel N.

AU - Villaseñor, Jesus Noel

AU - Vezie, Michael

AU - Lissauer, Jack J.

AU - Collins, Karen A.

AU - Collins, Kevin I.

AU - Isopi, Giovanni

AU - Mallia, Franco

AU - Ercolino, Andrea

AU - Petrovich, Cristobal

AU - Jordán, Andrés

AU - Acton, Jack S.

AU - Armstrong, David J.

AU - Bayliss, Daniel

AU - Bouchy, François

AU - Belardi, Claudia

AU - Bryant, Edward M.

AU - Burleigh, Matthew R.

AU - Cabrera, Juan

AU - Casewell, Sarah L.

AU - Chaushev, Alexander

AU - Cooke, Benjamin F.

AU - Eigmüller, Philipp

AU - Erikson, Anders

AU - Foxell, Emma

AU - Gänsicke, Boris T.

AU - Gill, Samuel

AU - Gillen, Edward

AU - Günther, Maximilian N.

AU - Goad, Michael R.

AU - Hooton, Matthew J.

AU - Jackman, James A.G.

AU - Louden, Tom

AU - McCormac, James

AU - Moyano, Maximiliano

AU - Nielsen, Louise D.

AU - Pollacco, Don

AU - Queloz, Didier

AU - Rauer, Heike

AU - Raynard, Liam

AU - Smith, Alexis M.S.

AU - Tilbrook, Rosanna H.

AU - Titz-Weider, Ruth

AU - Turner, Oliver

AU - Udry, Stéphane

AU - Walker, Simon R.

AU - Watson, Christopher A.

AU - West, Richard G.

AU - Palle, Enric

AU - Ziegler, Carl

AU - Law, Nicholas

AU - Mann, Andrew W.

PY - 2020/12

Y1 - 2020/12

N2 - About 1 out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultrashort-period planet1,2. All of the previously known ultrashort-period planets are either hot Jupiters, with sizes above 10 Earth radii (R⊕), or apparently rocky planets smaller than 2 R⊕. Such lack of planets of intermediate size (the ‘hot Neptune desert’) has been interpreted as the inability of low-mass planets to retain any hydrogen/helium (H/He) envelope in the face of strong stellar irradiation. Here we report the discovery of an ultrashort-period planet with a radius of 4.6 R⊕ and a mass of 29 M⊕, firmly in the hot Neptune desert. Data from the Transiting Exoplanet Survey Satellite3 revealed transits of the bright Sun-like star LTT 9779 every 0.79 days. The planet’s mean density is similar to that of Neptune, and according to thermal evolution models, it has a H/He-rich envelope constituting 9.0−2.9+2.7% of the total mass. With an equilibrium temperature around 2,000 K, it is unclear how this ‘ultrahot Neptune’ managed to retain such an envelope. Follow-up observations of the planet’s atmosphere to better understand its origin and physical nature will be facilitated by the star’s brightness (Vmag = 9.8).

AB - About 1 out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultrashort-period planet1,2. All of the previously known ultrashort-period planets are either hot Jupiters, with sizes above 10 Earth radii (R⊕), or apparently rocky planets smaller than 2 R⊕. Such lack of planets of intermediate size (the ‘hot Neptune desert’) has been interpreted as the inability of low-mass planets to retain any hydrogen/helium (H/He) envelope in the face of strong stellar irradiation. Here we report the discovery of an ultrashort-period planet with a radius of 4.6 R⊕ and a mass of 29 M⊕, firmly in the hot Neptune desert. Data from the Transiting Exoplanet Survey Satellite3 revealed transits of the bright Sun-like star LTT 9779 every 0.79 days. The planet’s mean density is similar to that of Neptune, and according to thermal evolution models, it has a H/He-rich envelope constituting 9.0−2.9+2.7% of the total mass. With an equilibrium temperature around 2,000 K, it is unclear how this ‘ultrahot Neptune’ managed to retain such an envelope. Follow-up observations of the planet’s atmosphere to better understand its origin and physical nature will be facilitated by the star’s brightness (Vmag = 9.8).

UR - http://www.scopus.com/inward/record.url?scp=85091611527&partnerID=8YFLogxK

U2 - 10.1038/s41550-020-1142-z

DO - 10.1038/s41550-020-1142-z

M3 - Article

AN - SCOPUS:85091611527

SN - 2397-3366

VL - 4

SP - 1148

EP - 1157

JO - Nature Astronomy

JF - Nature Astronomy

IS - 12

ER -

An ultrahot Neptune in the Neptune desert

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