Zobrazeno 1 - 10
of 91
pro vyhledávání: '"Eccentric Jupiter"'
Recent high precision meteoritic data improve constraints on the formation timescale and bulk composition of the terrestrial planets. High resolution N-body simulations allow direct comparison of embryo growth timescale and accretion zones to these c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ddeb5c2a2219366a6445982f99c04ebc
http://arxiv.org/abs/2101.09035
http://arxiv.org/abs/2101.09035
Publikováno v:
Physics of the Earth and Planetary Interiors. 269:40-57
Rocky exoplanets are typically classified as potentially habitable planets, if liquid water exists at the surface. The latter depends on several factors like the abundance of water but also on the amount of available solar energy and greenhouse gases
Publikováno v:
ResearcherID
With continued improvement in telescope sensitivity and observational techniques, the search for rocky planets in stellar habitable zones is entering an exciting era. With so many exoplanetary systems available for follow-up observations to find pote
Publikováno v:
Origins of Life and Evolution of Biospheres. 45:469-477
Approximately 60 percent of all stars in the solar neighbourhood (up to 80 percent in our Milky Way) are members of binary or multiple star systems. This fact led to the speculations that many more planets may exist in binary systems than are current
The Ru–Mo isotopic compositions of inner Solar System bodies may reflect the provenance of accreted material and how it evolved with time, both of which are controlled by the accretion scenario these bodies experienced. Here we use a total of 116 N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bba20d0a1f81f95dbe0359c36e6994a6
https://europepmc.org/articles/PMC5880038/
https://europepmc.org/articles/PMC5880038/
Autor:
J. J. Zanazzi, Dong Lai
Rocky planets orbiting M-dwarf stars in the habitable zone tend to be driven to synchronous rotation by tidal dissipation, potentially causing difficulties for maintaining a habitable climate on the planet. However, the planet may be captured into as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::761356fbfec812859019747ac9f97ad9
http://arxiv.org/abs/1702.07327
http://arxiv.org/abs/1702.07327
Autor:
Matthew S. Clement, Nathan A. Kaib
The formation of the solar system’s terrestrial planets has been numerically modeled in various works, and many other studies have been devoted to characterizing our modern planets’ chaotic dynamical state. However, it is still not known whether
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a1a22641b7ab8d5cc2f0ce27fa0f3fce
http://arxiv.org/abs/1701.07881
http://arxiv.org/abs/1701.07881
Autor:
Dong Lai, Kassandra R. Anderson
Recent studies have proposed that most warm Jupiters (WJs, giant planets with semi-major axes in the range of 0.1-1 AU) probably form in-situ, or arrive in their observed orbits through disk migration. However, both in-situ formation and disk migrati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1d2726f56fa0ea72a227d5d24601736
Autor:
Teriyuki Hirano, V. Wolthoff, Roi Alonso, A. P. Hatzes, Sz. Csizmadia, Norio Narita, Marshall C. Johnson, Felice Cusano, Judith Korth, Brendan P. Bowler, Juan Cabrera, Eike W. Guenther, Enric Palle, Heike Rauer, Simon Albrecht, Hans J. Deeg, Anders Erikson, Ph. Eigmüller, Michael Endl, Brandon Tingley, David Nespral, Andrew W. Mann, Alexis M. S. Smith, Martin Pätzold, Davide Gandolfi, Grzegorz Nowak, Jorge Prieto-Arranz, Sascha Grziwa, William D. Cochran, D. Hidalgo, Malcolm Fridlund, Oscar Barragán, Ignasi Ribas
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 464, 2708-2716
Smith, A M S, Gandolfi, D, Barragan, O, Bowler, B, Csizmadia, S, Endl, M, Fridlund, M C V, Grziwa, S, Guenther, E, Hatzes, A P, Nowak, G, Albrecht, S, Alonso, R, Cabrera, J, Cochran, W D, Deeg, H J, Cusano, F, Eigmueller, P, Erikson, A, Hidalgo, D, Hirano, T, Johnson, M C, Korth, J, Mann, A, Narita, N, Nespral, D, Palle, E, Paetzold, M, Prieto-Arranz, J, Rauer, H, Ribas, I, Tingley, B & Wolthoff, V 2017, ' K2-99 : a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion ', Royal Astronomical Society. Monthly Notices, vol. 464, no. 3, pp. 2708-2716 . https://doi.org/10.1093/mnras/stw2487
Smith, A M S, Gandolfi, D, Barragan, O, Bowler, B, Csizmadia, S, Endl, M, Fridlund, M C V, Grziwa, S, Guenther, E, Hatzes, A P, Nowak, G, Albrecht, S, Alonso, R, Cabrera, J, Cochran, W D, Deeg, H J, Cusano, F, Eigmueller, P, Erikson, A, Hidalgo, D, Hirano, T, Johnson, M C, Korth, J, Mann, A, Narita, N, Nespral, D, Palle, E, Paetzold, M, Prieto-Arranz, J, Rauer, H, Ribas, I, Tingley, B & Wolthoff, V 2017, ' K2-99 : a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion ', Royal Astronomical Society. Monthly Notices, vol. 464, no. 3, pp. 2708-2716 . https://doi.org/10.1093/mnras/stw2487
We report the discovery from K2 of a transiting planet in an 18.25-d, eccentric (0.19$\pm$ 0.04) orbit around K2-99, an 11th magnitude subgiant in Virgo. We confirm the planetary nature of the companion with radial velocities, and determine that the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3700e82c789c6f06d0c5dfc659c6ed14
http://hdl.handle.net/1887/59284
http://hdl.handle.net/1887/59284
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 442:454-461
Using numerical methods we investigate the dynamical stability of the Gliese 581 exoplanetary system. The system is known to harbour four planets (b-e). The existence of another planet (g) in the liquid water habitable zone of the star is debated aft