Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 b

Characterising the atmospheres of exoplanets is key to understanding their nature and provides hints about their formation and evolution. High resolution measurements of the helium triplet absorption of highly irradiated planets have been recently reported, which provide a new means of studying thei...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Lampón, Manuel (VerfasserIn) , López-Puertas, M. (VerfasserIn) , Sanz-Forcada, J. (VerfasserIn) , Sánchez-López, A. (VerfasserIn) , Molaverdikhani, Karan (VerfasserIn) , Czesla, S. (VerfasserIn) , Quirrenbach, Andreas (VerfasserIn) , Pallé, E. (VerfasserIn) , Caballero, J. A. (VerfasserIn) , Henning, Thomas (VerfasserIn) , Salz, M. (VerfasserIn) , Nortmann, L. (VerfasserIn) , Aceituno, J. (VerfasserIn) , Amado, P. J. (VerfasserIn) , Bauer, F. F. (VerfasserIn) , Montes, D. (VerfasserIn) , Nagel, E. (VerfasserIn) , Reiners, A. (VerfasserIn) , Ribas, I. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 23 March 2021
In: Astronomy and astrophysics
Year: 2021, Jahrgang: 647, Pages: 1-16
ISSN:1432-0746
DOI:10.1051/0004-6361/202039417
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/202039417
Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2021/03/aa39417-20/aa39417-20.html
Volltext
Verfasserangaben:M. Lampón, M. López-Puertas, J. Sanz-Forcada, A. Sánchez-López, K. Molaverdikhani, S. Czesla, A. Quirrenbach, E. Pallé, J.A. Caballero, T. Henning, M. Salz, L. Nortmann, J. Aceituno, P.J. Amado, F.F. Bauer, D. Montes, E. Nagel, A. Reiners, and I. Ribas

MARC

LEADER 00000caa a2200000 c 4500
001 1756670803
003 DE-627
005 20220819191659.0
007 cr uuu---uuuuu
008 210430s2021 xx |||||o 00| ||eng c
024 7 |a 10.1051/0004-6361/202039417  |2 doi 
035 |a (DE-627)1756670803 
035 |a (DE-599)KXP1756670803 
035 |a (OCoLC)1341407570 
040 |a DE-627  |b ger  |c DE-627  |e rda 
041 |a eng 
084 |a 29  |2 sdnb 
100 1 |a Lampón, Manuel  |e VerfasserIn  |0 (DE-588)1212122763  |0 (DE-627)1700734725  |4 aut 
245 1 0 |a Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 b  |c M. Lampón, M. López-Puertas, J. Sanz-Forcada, A. Sánchez-López, K. Molaverdikhani, S. Czesla, A. Quirrenbach, E. Pallé, J.A. Caballero, T. Henning, M. Salz, L. Nortmann, J. Aceituno, P.J. Amado, F.F. Bauer, D. Montes, E. Nagel, A. Reiners, and I. Ribas 
264 1 |c 23 March 2021 
300 |a 16 
336 |a Text  |b txt  |2 rdacontent 
337 |a Computermedien  |b c  |2 rdamedia 
338 |a Online-Ressource  |b cr  |2 rdacarrier 
500 |a Ångström, die Maßeinheit der Länge, wird im Text als A mit Ring dargestellt 
500 |a Gesehen am 30.04.2021 
520 |a Characterising the atmospheres of exoplanets is key to understanding their nature and provides hints about their formation and evolution. High resolution measurements of the helium triplet absorption of highly irradiated planets have been recently reported, which provide a new means of studying their atmospheric escape. In this work we study the escape of the upper atmospheres of HD 189733 b and GJ 3470 b by analysing high resolution He I triplet absorption measurements and using a 1D hydrodynamic spherically symmetric model coupled with a non-local thermodynamic model for the He I triplet state. We also use the H density derived from Ly<i>α<i/> observations to further constrain their temperatures, mass-loss rates, and H/He ratios. We have significantly improved our knowledge of the upper atmospheres of these planets. While HD 189733 b has a rather compressed atmosphere and small gas radial velocities, GJ 3470 b, on the other hand with a gravitational potential ten times smaller, exhibits a very extended atmosphere and large radial outflow velocities. Hence, although GJ 3470 b is much less irradiated in the X-ray and extreme ultraviolet radiation, and its upper atmosphere is much cooler, it evaporates at a comparable rate. In particular, we find that the upper atmosphere of HD 189733 b is compact and hot, with a maximum temperature of 12 400 K, with a very low mean molecular mass (H/He = (99.2/0.8) ± 0.1), which is almost fully ionised above 1.1 <i>R<i/><sub>P<sub/>, and with a mass-loss rate of (1.1 ± 0.1) × 10<sup>11<sup/> g s<sup>−1<sup/>. In contrast, the upper atmosphere of GJ 3470 b is highly extended and relatively cold, with a maximum temperature of 5100 ± 900 K, also with a very low mean molecular mass (H/He = (98.5/1.5) ), which is not strongly ionised, and with a mass-loss rate of (1.9 ± 1.1) × 10<sup>11<sup/> g s<sup>−1<sup/>. Furthermore, our results suggest that upper atmospheres of giant planets undergoing hydrodynamic escape tend to have a very low mean molecular mass (H/He ≳ 97/3). 
700 1 |a López-Puertas, M.  |e VerfasserIn  |4 aut 
700 1 |a Sanz-Forcada, J.  |e VerfasserIn  |4 aut 
700 1 |a Sánchez-López, A.  |e VerfasserIn  |4 aut 
700 1 |a Molaverdikhani, Karan  |d 1982-  |e VerfasserIn  |0 (DE-588)1205499784  |0 (DE-627)1691167576  |4 aut 
700 1 |a Czesla, S.  |e VerfasserIn  |4 aut 
700 1 |a Quirrenbach, Andreas  |e VerfasserIn  |0 (DE-588)112240623  |0 (DE-627)593634780  |0 (DE-576)304098167  |4 aut 
700 1 |a Pallé, E.  |e VerfasserIn  |4 aut 
700 1 |a Caballero, J. A.  |e VerfasserIn  |4 aut 
700 1 |a Henning, Thomas  |d 1956-  |e VerfasserIn  |0 (DE-588)124568637  |0 (DE-627)526967811  |0 (DE-576)294236120  |4 aut 
700 1 |a Salz, M.  |e VerfasserIn  |4 aut 
700 1 |a Nortmann, L.  |e VerfasserIn  |4 aut 
700 1 |a Aceituno, J.  |e VerfasserIn  |4 aut 
700 1 |a Amado, P. J.  |e VerfasserIn  |4 aut 
700 1 |a Bauer, F. F.  |e VerfasserIn  |4 aut 
700 1 |a Montes, D.  |e VerfasserIn  |4 aut 
700 1 |a Nagel, E.  |e VerfasserIn  |4 aut 
700 1 |a Reiners, A.  |e VerfasserIn  |4 aut 
700 1 |a Ribas, I.  |e VerfasserIn  |4 aut 
773 0 8 |i Enthalten in  |t Astronomy and astrophysics  |d Les Ulis : EDP Sciences, 1969  |g 647(2021), Artikel-ID A129, Seite 1-16  |h Online-Ressource  |w (DE-627)253390222  |w (DE-600)1458466-9  |w (DE-576)072283351  |x 1432-0746  |7 nnas  |a Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 b 
773 1 8 |g volume:647  |g year:2021  |g elocationid:A129  |g pages:1-16  |g extent:16  |a Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 b 
856 4 0 |u https://doi.org/10.1051/0004-6361/202039417  |x Verlag  |x Resolving-System  |z lizenzpflichtig  |3 Volltext 
856 4 0 |u https://www.aanda.org/articles/aa/abs/2021/03/aa39417-20/aa39417-20.html  |x Verlag  |z lizenzpflichtig  |3 Volltext 
951 |a AR 
992 |a 20210430 
993 |a Article 
994 |a 2021 
998 |g 124568637  |a Henning, Thomas  |m 124568637:Henning, Thomas  |d 130000  |e 130000PH124568637  |k 0/130000/  |p 10 
998 |g 112240623  |a Quirrenbach, Andreas  |m 112240623:Quirrenbach, Andreas  |d 700000  |d 714000  |d 714300  |e 700000PQ112240623  |e 714000PQ112240623  |e 714300PQ112240623  |k 0/700000/  |k 1/700000/714000/  |k 2/700000/714000/714300/  |p 7 
998 |g 1205499784  |a Molaverdikhani, Karan  |m 1205499784:Molaverdikhani, Karan  |d 700000  |d 714000  |d 714300  |e 700000PM1205499784  |e 714000PM1205499784  |e 714300PM1205499784  |k 0/700000/  |k 1/700000/714000/  |k 2/700000/714000/714300/  |p 5 
999 |a KXP-PPN1756670803  |e 392030019X 
BIB |a Y 
SER |a journal 
JSO |a {"language":["eng"],"id":{"eki":["1756670803"],"doi":["10.1051/0004-6361/202039417"]},"recId":"1756670803","title":[{"title":"Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 b","title_sort":"Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 b"}],"person":[{"role":"aut","given":"Manuel","family":"Lampón","display":"Lampón, Manuel"},{"display":"López-Puertas, M.","role":"aut","given":"M.","family":"López-Puertas"},{"display":"Sanz-Forcada, J.","family":"Sanz-Forcada","role":"aut","given":"J."},{"family":"Sánchez-López","given":"A.","role":"aut","display":"Sánchez-López, A."},{"family":"Molaverdikhani","role":"aut","given":"Karan","display":"Molaverdikhani, Karan"},{"display":"Czesla, S.","family":"Czesla","role":"aut","given":"S."},{"display":"Quirrenbach, Andreas","family":"Quirrenbach","role":"aut","given":"Andreas"},{"family":"Pallé","given":"E.","role":"aut","display":"Pallé, E."},{"display":"Caballero, J. A.","role":"aut","given":"J. A.","family":"Caballero"},{"given":"Thomas","role":"aut","family":"Henning","display":"Henning, Thomas"},{"family":"Salz","given":"M.","role":"aut","display":"Salz, M."},{"display":"Nortmann, L.","family":"Nortmann","given":"L.","role":"aut"},{"display":"Aceituno, J.","given":"J.","role":"aut","family":"Aceituno"},{"display":"Amado, P. J.","given":"P. J.","role":"aut","family":"Amado"},{"family":"Bauer","given":"F. F.","role":"aut","display":"Bauer, F. F."},{"display":"Montes, D.","family":"Montes","role":"aut","given":"D."},{"family":"Nagel","given":"E.","role":"aut","display":"Nagel, E."},{"display":"Reiners, A.","role":"aut","given":"A.","family":"Reiners"},{"role":"aut","given":"I.","family":"Ribas","display":"Ribas, I."}],"name":{"displayForm":["M. Lampón, M. López-Puertas, J. Sanz-Forcada, A. Sánchez-López, K. Molaverdikhani, S. Czesla, A. Quirrenbach, E. Pallé, J.A. Caballero, T. Henning, M. Salz, L. Nortmann, J. Aceituno, P.J. Amado, F.F. Bauer, D. Montes, E. Nagel, A. Reiners, and I. Ribas"]},"origin":[{"dateIssuedDisp":"23 March 2021","dateIssuedKey":"2021"}],"type":{"media":"Online-Ressource","bibl":"article-journal"},"note":["Ångström, die Maßeinheit der Länge, wird im Text als A mit Ring dargestellt","Gesehen am 30.04.2021"],"relHost":[{"titleAlt":[{"title":"Astronomy & astrophysics"},{"title":"a European journal"}],"id":{"eki":["253390222"],"zdb":["1458466-9"],"issn":["1432-0746"]},"recId":"253390222","disp":"Modelling the He I triplet absorption at 10 830 Å in the atmospheres of HD 189733 b and GJ 3470 bAstronomy and astrophysics","corporate":[{"role":"isb","display":"European Southern Observatory"}],"note":["Gesehen am 21.06.2024","Erscheint 36mal jährlich in 12 Bänden zu je 3 Ausgaben","Fortsetzung der Druck-Ausgabe"],"origin":[{"dateIssuedDisp":"1969-","publisher":"EDP Sciences ; Springer","publisherPlace":"Les Ulis ; Berlin ; Heidelberg","dateIssuedKey":"1969"}],"pubHistory":["1.1969 -"],"language":["eng"],"physDesc":[{"extent":"Online-Ressource"}],"title":[{"subtitle":"an international weekly journal","title_sort":"Astronomy and astrophysics","title":"Astronomy and astrophysics"}],"name":{"displayForm":["European Southern Observatory (ESO)"]},"part":{"pages":"1-16","volume":"647","text":"647(2021), Artikel-ID A129, Seite 1-16","extent":"16","year":"2021"},"type":{"media":"Online-Ressource","bibl":"periodical"}}],"physDesc":[{"extent":"16 S."}]} 
SRT |a LAMPONMANUMODELLINGT2320