Open AccessThe composition of the Jovian atmosphere as determined by the Galileo probe mass spectrometer
Author(s) -
Niemann H. B.,
Atreya S. K.,
Carignan G. R.,
Donahue T. M.,
Haberman J. A.,
Harpold D. N.,
Hartle R. E.,
Hunten D. M.,
Kasprzak W. T.,
Mahaffy P. R.,
Owen T. C.,
Way S. H.
Publication year - 1998
Publication title -
journal of geophysical research: planets
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/98je01050
Subject(s) - jovian , mixing ratio , atmosphere (unit) , atmosphere of jupiter , mixing (physics) , physics , jupiter (rocket family) , analytical chemistry (journal) , astrobiology , astrophysics , atmospheric sciences , chemistry , astronomy , meteorology , saturn , environmental chemistry , space shuttle , quantum mechanics , planet
The Galileo probe mass spectrometer determined the composition of the Jovian atmosphere for species with masses between 2 and 150 amu from 0.5 to 21.1 bars. This paper presents the results of analysis of some of the constituents detected: H 2 , He, Ne, Ar, Kr, Xe, CH 4 , NH 3 , H 2 O, H 2 S, C 2 and C 3 nonmethane hydrocarbons, and possibly PH 3 and Cl. 4 He/H 2 in the Jovian atmosphere was measured to be 0.157±0.030. 13 C/ 12 C was found to be 0.0108±0.0005, and D/H and 3 He/ 4 He were measured. Ne was depleted, ≤0.13 times solar, Ar ≤1.7 solar, Kr ≤5 solar, and Xe ≤5 solar. CH 4 has a constant mixing ratio of (2.1±0.4) × 10 −3 ( 12 C, 2.9 solar), where the mixing ratio is relative to H 2 . Upper limits to the H 2 O mixing ratio rose from 8 × 10 −7 at pressures <3.8 bars to (5.6±2.5) × 10 −5 ( 16 O, 0.033±0.015 solar) at 11.7 bars and, provisionally, about an order of magnitude larger at 18.7 bars. The mixing ratio of H 2 S was <10 −6 at pressures less than 3.8 bars but rose from about 0.7 × 10 −5 at 8.7 bars to about 7.7 × 10 −5 ( 32 S, 2.5 solar) above 15 bars. Only very large upper limits to the NH 3 mixing ratio have been set at present. If PH 3 and Cl were present, their mixing ratios also increased with pressure. Species were detected at mass peaks appropriate for C 2 and C 3 hydrocarbons. It is not yet clear which of these were atmospheric constituents and which were instrumentally generated. These measurements imply (1) fractionation of 4 He, (2) a local, altitude‐dependent depletion of condensables, probably because the probe entered the descending arm of a circulation cell, (3) that icy planetesimals made significant contributions to the volatile inventory, and (4) a moderate decrease in D/H but no detectable change in (D + 3 He)/H in this part of the galaxy during the past 4.6 Gyr.