Volatile-rich earth-mass planets in the habitable zone

被引：132

作者：

Kuchner, MJ ^{[1
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

来源：

ASTROPHYSICAL JOURNAL | 2003年 / 596卷 / 01期

基金：

美国国家航空航天局;

关键词：

astrobiology; planetary systems;

D O I：

10.1086/378397

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A small planet is not necessarily a terrestrial planet. Planets that form beyond the snow line with too little mass to seed rapid gas accretion (less than or similar to 10(+)) should be rich in volatile ices like H2O and NH3. Some of these planets should migrate inward by interacting with a circumstellar disk or with other planets. Such objects can retain their volatiles for billions of years or longer at similar to 1 AU as their thick steam atmospheres undergo slow hydrodynamic escape. These objects could appear in future surveys for extrasolar Earth analogs.

引用

页码：L105 / L108

页数：4

共 50 条

[21] The CARMENES search for exoplanets around M dwarfs Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star [J].

Kossakowski, D. ;

Kuerster, M. ;

Trifonov, T. ;

Henning, Th. ;

Kemmer, J. ;

Caballero, J. A. ;

Burn, R. ;

Sabotta, S. ;

Crouse, J. S. ;

Fauchez, T. J. ;

Nagel, E. ;

Kaminski, A. ;

Herrero, E. ;

Rodriguez, E. ;

Gonzalez-Alvarez, E. ;

Quirrenbach, A. ;

Amado, P. J. ;

Ribas, I. ;

Reiners, A. ;

Aceituno, J. ;

Bejar, V. J. S. ;

Baroch, D. ;

Bastelberger, S. T. ;

Chaturvedi, P. ;

Cifuentes, C. ;

Dreizler, S. ;

Jeffers, S. V. ;

Kopparapu, R. ;

Lafarga, M. ;

Lopez-Gonzalez, M. J. ;

Martin-Ruiz, S. ;

Montes, D. ;

Morales, J. C. ;

Palle, E. ;

Pavlov, A. ;

Pedraz, S. ;

Perdelwitz, V. ;

Perez-Torres, M. ;

Perger, M. ;

Reffert, S. ;

Rodriguez Lopez, C. ;

Schlecker, M. ;

Schoefer, P. ;

Schweitzer, A. ;

Shan, Y. ;

Shields, A. ;

Stock, S. ;

Wolf, E. ;

Zapatero Osorio, M. R. ;

Zechmeister, M. .

ASTRONOMY & ASTROPHYSICS, 2023, 670

[22] Additional planets in the habitable zone of Gliese 581? [J].

Zollinger, R. ;

Armstrong, J. C. .

ASTRONOMY & ASTROPHYSICS, 2009, 497 (02) :583-587

[23] The Impact of Stellar Distances on Habitable Zone Planets [J].

Kane, Stephen R. .

ASTROPHYSICAL JOURNAL LETTERS, 2018, 861 (02)

[24] THE RADIAL VELOCITY DETECTION OF EARTH-MASS PLANETS IN THE PRESENCE OF ACTIVITY NOISE: THE CASE OF α CENTAURI Bb [J].

Hatzes, Artie P. .

ASTROPHYSICAL JOURNAL, 2013, 770 (02)

[25] Searching for Earth-mass planets around α Centauri: precise radial velocities from contaminated spectra [J].

Bergmann, Christoph ;

Endl, Michael ;

Hearnshaw, John B. ;

Wittenmyer, Robert A. ;

Wright, Duncan J. .

INTERNATIONAL JOURNAL OF ASTROBIOLOGY, 2015, 14 (02) :173-176

[26] Sensitivity of transit searches to habitable-zone planets [J].

Gould, A ;

Pepper, J ;

DePoy, DL .

ASTROPHYSICAL JOURNAL, 2003, 594 (01) :533-537

[27] Tidal excitation of the obliquity of Earth-like planets in the habitable zone of M-dwarf stars [J].

Valente, Ema F. S. ;

Correia, Alexandre C. M. .

ASTRONOMY & ASTROPHYSICS, 2022, 665

[28] The HARPS search for Earth-like planets in the habitable zone I. Very low-mass planets around HD 20794, HD 85512, and HD 192310 [J].

Pepe, F. ;

Lovis, C. ;

Segransan, D. ;

Benz, W. ;

Bouchy, F. ;

Dumusque, X. ;

Mayor, M. ;

Queloz, D. ;

Santos, N. C. ;

Udry, S. .

ASTRONOMY & ASTROPHYSICS, 2011, 534

[29] The influence of giant planets near a mean motion resonance on earth-like planets in the habitable zone of Sun-like stars [J].

Pilat-Lohinger, E. ;

Sueli, A. ;

Robutel, P. ;

Freistetter, F. .

ASTROPHYSICAL JOURNAL, 2008, 681 (02) :1639-1645

[30] Ocean Dynamics and the Inner Edge of the Habitable Zone for Tidally Locked Terrestrial Planets [J].

Yang, Jun ;

Abbot, Dorian S. ;

Koll, Daniel D. B. ;

Hu, Yongyun ;

Showman, Adam P. .

ASTROPHYSICAL JOURNAL, 2019, 871 (01)

← 1 2 3 4 5 →