High-resolution 10-micronmeter spectroscopy of ammonia and phosphine lines on Jupiter

被引:47
|
作者
Lara, LM [1 ]
Bezard, B
Griffith, CA
Lacy, JH
Owen, T
机构
[1] Observ Paris, Meudon Sect, Dept Rech Spatiale, F-92195 Meudon, France
[2] No Arizona Univ, Dept Phys & Astron, Flagstaff, AZ 86011 USA
[3] Univ Texas, Dept Astron, Austin, TX 78712 USA
[4] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[5] Inst Astrofis Andalucia, E-18080 Granada, Spain
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
Jupiter; atmosphere; atmospheres; composition; structure; infrared observations;
D O I
10.1006/icar.1997.5868
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High spectral resolution measurements of NH3 and PH3 lines on Jupiter in the 10.5- to 11.2-mu m range are presented, Observations, recorded on January 21-23, 1991, cover the 10 degrees-40 degrees S latitude range and several longitudes including the Great Red Spot (GRS), Information on the temperature in the upper troposphere was retrieved from the continuum radiance at wavelengths around 12.8 and 17.8 Ecm. At all observed longitudes, the 200-mbar temperature field is minimum at latitudes of 20 degrees-25 degrees S near the location of the South Tropical Zone, in agreement with Voyager infrared retrievals, This minimum temperature is lower over the GRS than at other longitudes, The ammonia mixing ratio at similar to 380 mbar is not significantly enhanced over the GRS. The phosphine abundance probed at similar to 580 mbar is also not enhanced (within a precision of 10%), suggesting that this molecule is not a precursor of the reddish chromophores, The NH3 abundance at 380 mbar varies highly with latitude and longitude, a possible consequence of the active jovian meteorology, At the resolution of our observations (similar to 8000 km), the NH3 humidity at this altitude ranges between 15 and 100% throughout the available data set. Above the cloud tops, the NH, mixing ratio in the 240-mbar region reaches a maximum near 15 degrees-18 degrees S and decreases by a factor of similar to 40 at latitudes 30 degrees-35 degrees S. This variation is not correlated with the 200-mbar temperature. It can be explained by a decrease of the eddy mixing coefficient near 240 mbar from similar to 4000 to less than or equal to 400 cm(2) sec(-1) between the two latitude ranges, The PH3 mixing ratio near 580 mbar lies between 1.7 and 2.6 x 10(-7) in the observed regions. At all longitudes, PH3 varies smoothly with latitude, decreasing by similar to 30% from 10 degrees to 35 degrees S. This variation may also reflect a decrease in the strength of the eddy mixing near 580 mbar or at deeper levels in the atmosphere. (C) 1998 Academic Press.
引用
收藏
页码:317 / 333
页数:17
相关论文
共 50 条
  • [21] HIGH-RESOLUTION SPECTRA OF JUPITER NORTHERN AURORAL ULTRAVIOLET EMISSION WITH THE HUBBLE-SPACE-TELESCOPE
    TRAFTON, LM
    GERARD, JC
    MUNHOVEN, G
    WAITE, JH
    ASTROPHYSICAL JOURNAL, 1994, 421 (02) : 816 - 827
  • [22] The Internal Structure and Dynamics of Jupiter Unveiled by a High-Resolution Magnetic Field and Secular Variation Model
    Sharan, S.
    Langlais, B.
    Amit, H.
    Thebault, E.
    Pinceloup, M.
    Verhoeven, O.
    GEOPHYSICAL RESEARCH LETTERS, 2022, 49 (15)
  • [23] Detection and characterization of Io's atmosphere from high-resolution 4-μm spectroscopy
    Lellouch, E.
    Ali-Dib, M.
    Jessup, K. -L.
    Smette, A.
    Kaeufl, H. -U.
    Marchis, F.
    ICARUS, 2015, 253 : 99 - 114
  • [24] Spatial variations of the sodium/potassium ratio in Mercury's exosphere uncovered by high-resolution spectroscopy
    Doressoundiram, A.
    Leblanc, F.
    Foellmi, C.
    Gicquel, A.
    Cremonese, G.
    Donati, J. -F.
    Veillet, C.
    ICARUS, 2010, 207 (01) : 1 - 8
  • [25] Fresh view of the hot brown dwarf HD 984 B through high-resolution spectroscopy
    Costes, J. C.
    Xuan, J. W.
    Vigan, A.
    Wang, J.
    D'Orazi, V.
    Molliere, P.
    Baker, A.
    Bartos, R.
    Blake, G. A.
    Calvin, B.
    Cetre, S.
    Delorme, J.
    Doppmann, G.
    Echeveri, D.
    Finnerty, L.
    Fitzgerald, M. P.
    Hsu, C.
    Jovanovic, N.
    Lopez, R.
    Mawet, D.
    Morris, E.
    Pezzato, J.
    Phillips, C. L.
    Ruffio, J.
    Sappey, B.
    Schneeberger, A.
    Schofield, T.
    Skemer, A. J.
    Wallace, J. K.
    Wang, J.
    ASTRONOMY & ASTROPHYSICS, 2024, 686
  • [26] κ Andromedae b Is a Fast Rotator from KPIC High-resolution Spectroscopy
    Morris, Evan C.
    Wang, Jason J.
    Hsu, Chih-Chun
    Ruffio, Jean-Baptiste
    Xuan, Jerry W.
    Delorme, Jacques-Robert
    Hood, Callie
    Bryan, Marta L.
    Martin, Emily C.
    Pezzato, Jacklyn
    Mawet, Dimitri
    Skemer, Andrew
    Baker, Ashley
    Bartos, Randall
    Calvin, Benjamin
    Cetre, Sylvain
    Doppmann, Greg
    Echeverri, Daniel
    Finnerty, Luke
    Fitzgerald, Michael P.
    Jovanovic, Nemanja
    Liberman, Joshua
    Lopez, Ronald
    Sappey, Ben
    Schofield, Tobias
    Wallace, J. Kent
    Wang, Ji
    ASTRONOMICAL JOURNAL, 2024, 168 (04)
  • [27] Feasibility of High-resolution Transmission Spectroscopy for Low-velocity Exoplanets
    Cheverall, Connor J.
    Madhusudhan, Nikku
    ASTRONOMICAL JOURNAL, 2024, 167 (06)
  • [28] High-resolution spectroscopy of R CrB - Pulsations, shells and mass loss
    Rao, NK
    Lambert, DL
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 284 (02) : 489 - 498
  • [29] On the synergy between Ariel and ground-based high-resolution spectroscopy
    Guilluy, Gloria
    Sozzetti, Alessandro
    Giacobbe, Paolo
    Bonomo, Aldo S.
    Micela, Giuseppina
    EXPERIMENTAL ASTRONOMY, 2022, 53 (02) : 655 - 677
  • [30] High-resolution optical spectroscopy of V838 Monocerotis in 2009
    Tylenda, R.
    Kaminski, T.
    Schmidt, M.
    Kurtev, R.
    Tomov, T.
    ASTRONOMY & ASTROPHYSICS, 2011, 532