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
  • [31] High-resolution transmission spectroscopy of MASCARA-2 b with EXPRES
    Hoeijmakers, H. Jens
    Cabot, Samuel H. C.
    Zhao, Lily
    Buchhave, Lars A.
    Tronsgaard, Rene
    Davis, Allen B.
    Kitzmann, Daniel
    Grimm, Simon L.
    Cegla, Heather M.
    Bourrier, Vincent
    Ehrenreich, David
    Heng, Kevin
    Lovis, Christophe
    Fischer, Debra A.
    ASTRONOMY & ASTROPHYSICS, 2020, 641 (641)
  • [32] High-resolution 3-μm spectra of Jupiter: Latitudinal spectral variations influenced by molecules, clouds, and haze
    Kim, Sang J.
    Geballe, T. R.
    Kim, J. H.
    Jung, A.
    Seo, H. J.
    Minh, Y. C.
    ICARUS, 2010, 208 (02) : 837 - 849
  • [33] ExoGemS High-resolution Transmission Spectroscopy of WASP-76b with GRACES
    Deibert, Emily K.
    de Mooij, Ernst J. W.
    Jayawardhana, Ray
    Turner, Jake D.
    Ridden-Harper, Andrew
    Hood, Callie E.
    Fortney, Jonathan J.
    Flagg, Laura
    Fossati, Luca
    Allart, Romain
    Brogi, Matteo
    MacDonald, Ryan J.
    ASTRONOMICAL JOURNAL, 2023, 166 (04)
  • [34] High-resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b
    Ridden-Harper, Andrew
    Nugroho, Stevanus K.
    Flagg, Laura
    Jayawardhana, Ray
    Turner, Jake D.
    de Mooij, Ernst
    MacDonald, Ryan
    Deibert, Emily
    Tamura, Motohide
    Kotani, Takayuki
    Hirano, Teruyuki
    Kuzuhara, Masayuki
    Omiya, Masashi
    Kusakabe, Nobuhiko
    ASTRONOMICAL JOURNAL, 2023, 165 (04)
  • [35] Prospects for Characterizing the Haziest Sub-Neptune Exoplanets with High-resolution Spectroscopy
    Hood, Callie E.
    Fortney, Jonathan J.
    Line, Michael R.
    Martin, Emily C.
    Morley, Caroline V.
    Birkby, Jayne L.
    Rustamkulov, Zafar
    Lupu, Roxana E.
    Freedman, Richard S.
    ASTRONOMICAL JOURNAL, 2020, 160 (05)
  • [36] Study of the sedge (Carex) lignin by high-resolution mass spectrometry and NMR spectroscopy
    Pikovskoi, I. I.
    Kosyakov, D. S.
    Faleva, A., V
    Shavrina, I. S.
    Kozhevnikov, A. Yu
    Ul'yanovskii, N., V
    RUSSIAN CHEMICAL BULLETIN, 2020, 69 (10) : 2004 - 2012
  • [37] High-resolution Transmission Spectroscopy of Four Hot Inflated Gas Giant Exoplanets
    Zak, Jiri
    Kabath, Petr
    Boffin, Henri M. J.
    Ivanov, Valentin D.
    Skarka, Marek
    ASTRONOMICAL JOURNAL, 2019, 158 (03)
  • [38] Robustness measures for molecular detections using high-resolution transmission spectroscopy of exoplanets
    Cheverall, Connor J.
    Madhusudhan, Nikku
    Holmberg, Mans
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 522 (01) : 661 - 677
  • [39] High-resolution Transmission Spectroscopy of Warm Jupiters: An ESPRESSO Sample with Predictions for ANDES
    Prinoth, Bibiana
    Sedaghati, Elyar
    Seidel, Julia V.
    Hoeijmakers, H. Jens
    Brahm, Rafael
    Thorsbro, Brian
    Jordan, Andres
    ASTRONOMICAL JOURNAL, 2024, 168 (03)
  • [40] DETERMINATION OF THE MOLECULAR-STRUCTURE OF DIACETYLENE FROM HIGH-RESOLUTION FTIR SPECTROSCOPY
    TAY, R
    METHA, GF
    SHANKS, F
    MCNAUGHTON, D
    STRUCTURAL CHEMISTRY, 1995, 6 (01) : 47 - 55