Volatile transport modeling on Triton with new observational constraints

Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby...
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Autor*in:	Bertrand, T. [verfasserIn] Lellouch, E. [verfasserIn] Holler, B.J. [verfasserIn] Young, L.A. [verfasserIn] Schmitt, B. [verfasserIn] Marques Oliveira, J. [verfasserIn] Sicardy, B. [verfasserIn] Forget, F. [verfasserIn] Grundy, W.M. [verfasserIn] Merlin, F. [verfasserIn] Vangvichith, M. [verfasserIn] Millour, E. [verfasserIn] Schenk, P.M. [verfasserIn] Hansen, C.J. [verfasserIn] White, O.L. [verfasserIn] Moore, J.M. [verfasserIn] Stansberry, J.A. [verfasserIn] Oza, A.V. [verfasserIn] Dubois, D. [verfasserIn] Quirico, E. [verfasserIn] Cruikshank, D.P. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2021

Schlagwörter:	Triton Volatile transport Surface Modeling JWST

Übergeordnetes Werk:	Enthalten in: Icarus - Orlando, Fla. : Academ. Press, 1962, 373
Übergeordnetes Werk:	volume:373

DOI / URN:	10.1016/j.icarus.2021.114764

Katalog-ID:	ELV007078099

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520			\|a Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate.
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700	1		\|a Schmitt, B. \|e verfasserin \|4 aut
700	1		\|a Marques Oliveira, J. \|e verfasserin \|4 aut
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700	1		\|a Vangvichith, M. \|e verfasserin \|4 aut
700	1		\|a Millour, E. \|e verfasserin \|4 aut
700	1		\|a Schenk, P.M. \|e verfasserin \|4 aut
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700	1		\|a Moore, J.M. \|e verfasserin \|4 aut
700	1		\|a Stansberry, J.A. \|e verfasserin \|4 aut
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700	1		\|a Quirico, E. \|e verfasserin \|4 aut
700	1		\|a Cruikshank, D.P. \|e verfasserin \|4 aut
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allfields	10.1016/j.icarus.2021.114764 doi (DE-627)ELV007078099 (ELSEVIER)S0019-1035(21)00416-4 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bertrand, T. verfasserin aut Volatile transport modeling on Triton with new observational constraints 2021 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate. Triton Volatile transport Surface Modeling JWST Lellouch, E. verfasserin aut Holler, B.J. verfasserin aut Young, L.A. verfasserin aut Schmitt, B. verfasserin aut Marques Oliveira, J. verfasserin aut Sicardy, B. verfasserin aut Forget, F. verfasserin aut Grundy, W.M. verfasserin aut Merlin, F. verfasserin aut Vangvichith, M. verfasserin aut Millour, E. verfasserin aut Schenk, P.M. verfasserin aut Hansen, C.J. verfasserin aut White, O.L. verfasserin aut Moore, J.M. verfasserin aut Stansberry, J.A. verfasserin aut Oza, A.V. verfasserin aut Dubois, D. verfasserin aut Quirico, E. verfasserin aut Cruikshank, D.P. verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 373 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:373 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines VZ AR 373
spelling	10.1016/j.icarus.2021.114764 doi (DE-627)ELV007078099 (ELSEVIER)S0019-1035(21)00416-4 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bertrand, T. verfasserin aut Volatile transport modeling on Triton with new observational constraints 2021 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate. Triton Volatile transport Surface Modeling JWST Lellouch, E. verfasserin aut Holler, B.J. verfasserin aut Young, L.A. verfasserin aut Schmitt, B. verfasserin aut Marques Oliveira, J. verfasserin aut Sicardy, B. verfasserin aut Forget, F. verfasserin aut Grundy, W.M. verfasserin aut Merlin, F. verfasserin aut Vangvichith, M. verfasserin aut Millour, E. verfasserin aut Schenk, P.M. verfasserin aut Hansen, C.J. verfasserin aut White, O.L. verfasserin aut Moore, J.M. verfasserin aut Stansberry, J.A. verfasserin aut Oza, A.V. verfasserin aut Dubois, D. verfasserin aut Quirico, E. verfasserin aut Cruikshank, D.P. verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 373 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:373 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines VZ AR 373
allfields_unstemmed	10.1016/j.icarus.2021.114764 doi (DE-627)ELV007078099 (ELSEVIER)S0019-1035(21)00416-4 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bertrand, T. verfasserin aut Volatile transport modeling on Triton with new observational constraints 2021 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate. Triton Volatile transport Surface Modeling JWST Lellouch, E. verfasserin aut Holler, B.J. verfasserin aut Young, L.A. verfasserin aut Schmitt, B. verfasserin aut Marques Oliveira, J. verfasserin aut Sicardy, B. verfasserin aut Forget, F. verfasserin aut Grundy, W.M. verfasserin aut Merlin, F. verfasserin aut Vangvichith, M. verfasserin aut Millour, E. verfasserin aut Schenk, P.M. verfasserin aut Hansen, C.J. verfasserin aut White, O.L. verfasserin aut Moore, J.M. verfasserin aut Stansberry, J.A. verfasserin aut Oza, A.V. verfasserin aut Dubois, D. verfasserin aut Quirico, E. verfasserin aut Cruikshank, D.P. verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 373 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:373 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines VZ AR 373
allfieldsGer	10.1016/j.icarus.2021.114764 doi (DE-627)ELV007078099 (ELSEVIER)S0019-1035(21)00416-4 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bertrand, T. verfasserin aut Volatile transport modeling on Triton with new observational constraints 2021 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate. Triton Volatile transport Surface Modeling JWST Lellouch, E. verfasserin aut Holler, B.J. verfasserin aut Young, L.A. verfasserin aut Schmitt, B. verfasserin aut Marques Oliveira, J. verfasserin aut Sicardy, B. verfasserin aut Forget, F. verfasserin aut Grundy, W.M. verfasserin aut Merlin, F. verfasserin aut Vangvichith, M. verfasserin aut Millour, E. verfasserin aut Schenk, P.M. verfasserin aut Hansen, C.J. verfasserin aut White, O.L. verfasserin aut Moore, J.M. verfasserin aut Stansberry, J.A. verfasserin aut Oza, A.V. verfasserin aut Dubois, D. verfasserin aut Quirico, E. verfasserin aut Cruikshank, D.P. verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 373 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:373 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines VZ AR 373
allfieldsSound	10.1016/j.icarus.2021.114764 doi (DE-627)ELV007078099 (ELSEVIER)S0019-1035(21)00416-4 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bertrand, T. verfasserin aut Volatile transport modeling on Triton with new observational constraints 2021 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate. Triton Volatile transport Surface Modeling JWST Lellouch, E. verfasserin aut Holler, B.J. verfasserin aut Young, L.A. verfasserin aut Schmitt, B. verfasserin aut Marques Oliveira, J. verfasserin aut Sicardy, B. verfasserin aut Forget, F. verfasserin aut Grundy, W.M. verfasserin aut Merlin, F. verfasserin aut Vangvichith, M. verfasserin aut Millour, E. verfasserin aut Schenk, P.M. verfasserin aut Hansen, C.J. verfasserin aut White, O.L. verfasserin aut Moore, J.M. verfasserin aut Stansberry, J.A. verfasserin aut Oza, A.V. verfasserin aut Dubois, D. verfasserin aut Quirico, E. verfasserin aut Cruikshank, D.P. verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 373 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:373 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines VZ AR 373
language	English
source	Enthalten in Icarus 373 volume:373
sourceStr	Enthalten in Icarus 373 volume:373
format_phy_str_mv	Article
bklname	Sonnensystem: Allgemeines
institution	findex.gbv.de
topic_facet	Triton Volatile transport Surface Modeling JWST
dewey-raw	520
isfreeaccess_bool	false
container_title	Icarus
authorswithroles_txt_mv	Bertrand, T. @@aut@@ Lellouch, E. @@aut@@ Holler, B.J. @@aut@@ Young, L.A. @@aut@@ Schmitt, B. @@aut@@ Marques Oliveira, J. @@aut@@ Sicardy, B. @@aut@@ Forget, F. @@aut@@ Grundy, W.M. @@aut@@ Merlin, F. @@aut@@ Vangvichith, M. @@aut@@ Millour, E. @@aut@@ Schenk, P.M. @@aut@@ Hansen, C.J. @@aut@@ White, O.L. @@aut@@ Moore, J.M. @@aut@@ Stansberry, J.A. @@aut@@ Oza, A.V. @@aut@@ Dubois, D. @@aut@@ Quirico, E. @@aut@@ Cruikshank, D.P. @@aut@@
publishDateDaySort_date	2021-01-01T00:00:00Z
hierarchy_top_id	266881521
dewey-sort	3520
id	ELV007078099
language_de	englisch
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author	Bertrand, T.
spellingShingle	Bertrand, T. ddc 520 bkl 39.50 misc Triton misc Volatile transport misc Surface misc Modeling misc JWST Volatile transport modeling on Triton with new observational constraints
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topic_title	520 530 VZ 39.50 bkl Volatile transport modeling on Triton with new observational constraints Triton Volatile transport Surface Modeling JWST
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title	Volatile transport modeling on Triton with new observational constraints
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title_full	Volatile transport modeling on Triton with new observational constraints
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author_browse	Bertrand, T. Lellouch, E. Holler, B.J. Young, L.A. Schmitt, B. Marques Oliveira, J. Sicardy, B. Forget, F. Grundy, W.M. Merlin, F. Vangvichith, M. Millour, E. Schenk, P.M. Hansen, C.J. White, O.L. Moore, J.M. Stansberry, J.A. Oza, A.V. Dubois, D. Quirico, E. Cruikshank, D.P.
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title_sort	volatile transport modeling on triton with new observational constraints
title_auth	Volatile transport modeling on Triton with new observational constraints
abstract	Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate.
abstractGer	Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate.
abstract_unstemmed	Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich Kuiper Belt objects. The observations of Pluto by New Horizons acquired during the 2015 flyby and their analysis with volatile transport models (VTMs) shed light on how volatile sublimation-condensation cycles control the climate and shape the surface of such objects. Within the context of New Horizons observations as well as recent Earth-based observations of Triton, we adapt a Plutonian VTM to Triton, and test its ability to simulate its volatile cycles, thereby aiding our understanding of its climate.
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title_short	Volatile transport modeling on Triton with new observational constraints
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author2	Lellouch, E. Holler, B.J. Young, L.A. Schmitt, B. Marques Oliveira, J. Sicardy, B. Forget, F. Grundy, W.M. Merlin, F. Vangvichith, M. Millour, E. Schenk, P.M. Hansen, C.J. White, O.L. Moore, J.M. Stansberry, J.A. Oza, A.V. Dubois, D. Quirico, E. Cruikshank, D.P.
author2Str	Lellouch, E. Holler, B.J. Young, L.A. Schmitt, B. Marques Oliveira, J. Sicardy, B. Forget, F. Grundy, W.M. Merlin, F. Vangvichith, M. Millour, E. Schenk, P.M. Hansen, C.J. White, O.L. Moore, J.M. Stansberry, J.A. Oza, A.V. Dubois, D. Quirico, E. Cruikshank, D.P.
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doi_str	10.1016/j.icarus.2021.114764
up_date	2024-07-06T23:32:36.894Z
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Volatile transport modeling on Triton with new observational constraints

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