The Jupiter mass, also called Jovian mass, is the unit of mass equal to the total mass of the planet Jupiter. This value may refer to the mass of the planet alone, or the mass of the entire Jovian system to include the moons of Jupiter. Jupiter is by far the most massive planet in the Solar System. It is approximately 2.5 times as massive as all of the other planets in the Solar System combined.
Jupiter mass | |
---|---|
Relative masses of the giant planets of the outer Solar System | |
General information | |
Unit system | Astronomical system of units |
Unit of | mass |
Symbol | MJ, MJup or M♃ |
Conversions | |
1 MJin ... | ... is equal to ... |
SI base unit | (1.89813±0.00019)×1027 kg |
U.S. customary | ≈ 4.1847×1027 pounds |
Jupiter mass is a common unit of mass in astronomy that is used to indicate the masses of other similarly-sized objects, including the outer planets, extrasolar planets, and brown dwarfs, as this unit provides a convenient scale for comparison.
Current best estimates
The current best known value for the mass of Jupiter can be expressed as 1898130 yottagrams:
which is about 1⁄1000 as massive as the Sun (is about 0.1% M☉):
Jupiter is 318 times as massive as Earth:
Context and implications
Jupiter's mass is 2.5 times that of all the other planets in the Solar System combined—this is so massive that its barycenter with the Sun lies beyond the Sun's surface at 1.068 solar radii from the Sun's center.
Because the mass of Jupiter is so large compared to the other objects in the Solar System, the effects of its gravity must be included when calculating satellite trajectories and the precise orbits of other bodies in the Solar System, including the Moon and even Pluto.
Theoretical models indicate that if Jupiter had much more mass than it does at present, its atmosphere would collapse, and the planet would shrink. For small changes in mass, the radius would not change appreciably, but above about 500 ME (1.6 Jupiter masses) the interior would become so much more compressed under the increased pressure that its volume would decrease despite the increasing amount of matter. As a result, Jupiter is thought to have about as large a diameter as a planet of its composition and evolutionary history can achieve. The process of further shrinkage with increasing mass would continue until appreciable stellar ignition was achieved, as in high-mass brown dwarfs having around 50 Jupiter masses. Jupiter would need to be about 80 times as massive to fuse hydrogen and become a star.
Gravitational constant
The mass of Jupiter is derived from the measured value called the Jovian mass parameter, which is denoted with GMJ. The mass of Jupiter is calculated by dividing GMJ by the constant G. For celestial bodies such as Jupiter, Earth and the Sun, the value of the GM product is known to many orders of magnitude more precisely than either factor independently. The limited precision available for G limits the uncertainty of the derived mass. For this reason, astronomers often prefer to refer to the gravitational parameter, rather than the explicit mass. The GM products are used when computing the ratio of Jupiter mass relative to other objects.
In 2015, the International Astronomical Union defined the nominal Jovian mass parameter to remain constant regardless of subsequent improvements in measurement precision of MJ. This constant is defined as exactly
If the explicit mass of Jupiter is needed in SI units, it can be calculated by dividing GM by G, where G is the gravitational constant.
Mass composition
The majority of Jupiter's mass is hydrogen and helium. These two elements make up more than 87% of the total mass of Jupiter. The total mass of heavy elements other than hydrogen and helium in the planet is between 11 and 45 ME. The bulk of the hydrogen on Jupiter is solid hydrogen. Evidence suggests that Jupiter contains a central dense core. If so, the mass of the core is predicted to be no larger than about 12 ME. The exact mass of the core is uncertain due to the relatively poor knowledge of the behavior of solid hydrogen at very high pressures.
Relative mass
Object | MJ / Mobject | Mobject / MJ | Ref. |
---|---|---|---|
Sun | 9.547919(15)×10−4 | 1047.348644(17) | |
Earth | 317.82838 | 0.0031463520 | |
Jupiter | 1 | 1 | by definition |
Saturn | 3.3397683 | 0.29942197 | |
Uranus | 21.867552 | 0.045729856 | |
Neptune | 18.53467 | 0.05395295 | |
Gliese 229B | 21–52.4 | ||
51 Pegasi b | 0.472±0.039 |
See also
- Jupiter radius
- Hot Jupiter
- Orders of magnitude (mass)
- Planetary mass
- Solar mass
Notes
- Some of the values in this table are nominal values, derived from Numerical Standards for Fundamental Astronomy and rounded using appropriate attention to significant figures, as recommended by the IAU Resolution B3.
References
- "Planets and Pluto: Physical Characteristics". ssd.jpl.nasa.gov. Jet Propulsion Labritory. Retrieved 31 October 2017.
- Coffey, Jerry (18 June 2008). "Mass of Jupiter". Universe Today. Retrieved 2017-10-31.
- "Numerical Standards for Fundamental Astronomy". maia.usno.navy.mil. IAU Working Group. Archived from the original on 26 August 2016. Retrieved 31 October 2017.
- MacDougal, Douglas W. (November 6, 2012). "A Binary System Close to Home: How the Moon and Earth Orbit Each Other". Newton's Gravity. Undergraduate Lecture Notes in Physics. Springer New York. pp. 193–211. doi:10.1007/978-1-4614-5444-1_10. ISBN 9781461454434.
the barycenter is 743,000 km from the center of the sun. The Sun's radius is 696,000 km, so it is 47,000 km above the surface.
- Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. (2007). "Mass-Radius Relationships for Solid Exoplanets". The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390.
- How the Universe Works 3. Vol. Jupiter: Destroyer or Savior?. Discovery Channel. 2014.
- Guillot, Tristan (1999). "Interiors of Giant Planets Inside and Outside the Solar System". Science. 286 (5437): 72–77. Bibcode:1999Sci...286...72G. doi:10.1126/science.286.5437.72. PMID 10506563.
- Burrows, Adam; Hubbard, William B.; Saumon, D.; Lunine, Jonathan I. (1993). "An expanded set of brown dwarf and very low mass star models". Astrophysical Journal. 406 (1): 158–71. Bibcode:1993ApJ...406..158B. doi:10.1086/172427.
- Mamajek, E. E.; Prsa, A.; Torres, G.; et al. (2015). "IAU 2015 Resolution B3 on Recommended Nominal Conversion Constants for Selected Solar and Planetary Properties". arXiv:1510.07674 [astro-ph.SR].
- Guillot, Tristan; Stevenson, David J.; Hubbard, William B.; Saumon, Didier. "The Interior of Jupiter" (PDF). Retrieved 31 October 2017.
- Guillot, Tristan; Gautier, Daniel; Hubbard, William B. (December 1997). "New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models". Icarus. 130 (2): 534–539. arXiv:astro-ph/9707210. Bibcode:1997Icar..130..534G. doi:10.1006/icar.1997.5812. S2CID 5466469.
- Öpik, E. J. (January 1962). "Jupiter: Chemical composition, structure, and origin of a giant planet". Icarus. 1 (1–6): 200–257. Bibcode:1962Icar....1..200O. doi:10.1016/0019-1035(62)90022-2.
- "Planetary Fact Sheet – Ratio to Earth". nssdc.gsfc.nasa.gov. Retrieved 2016-02-12.
- White, Stephen M.; Jackson, Peter D.; Kundu, Mukul R. (December 1989). "A VLA survey of nearby flare stars". Astrophysical Journal Supplement Series. 71: 895–904. Bibcode:1989ApJS...71..895W. doi:10.1086/191401.
- Martins, J. H. C.; Santos, N. C.; Figueira, P.; et al. (2015). "Evidence for a spectroscopic direct detection of reflected light from 51 Peg b". Astronomy & Astrophysics. 576 (2015): A134. arXiv:1504.05962. Bibcode:2015A&A...576A.134M. doi:10.1051/0004-6361/201425298. S2CID 119224213.
The Jupiter mass also called Jovian mass is the unit of mass equal to the total mass of the planet Jupiter This value may refer to the mass of the planet alone or the mass of the entire Jovian system to include the moons of Jupiter Jupiter is by far the most massive planet in the Solar System It is approximately 2 5 times as massive as all of the other planets in the Solar System combined Jupiter massRelative masses of the giant planets of the outer Solar SystemGeneral informationUnit systemAstronomical system of unitsUnit ofmassSymbolMJ MJup or M Conversions1 MJin is equal to SI base unit 1 89813 0 00019 1027 kg U S customary 4 1847 1027 pounds Jupiter mass is a common unit of mass in astronomy that is used to indicate the masses of other similarly sized objects including the outer planets extrasolar planets and brown dwarfs as this unit provides a convenient scale for comparison Current best estimatesThe current best known value for the mass of Jupiter can be expressed as 1898 130 yottagrams MJ 1 89813 0 00019 1027 kg displaystyle M mathrm J 1 89813 pm 0 00019 times 10 27 text kg which is about 1 1000 as massive as the Sun is about 0 1 M MJ 11047 348644 0 000017M 9 547919 0 000002 10 4M displaystyle M mathrm J frac 1 1047 348644 pm 0 000017 M odot approx 9 547919 pm 0 000002 times 10 4 M odot Jupiter is 318 times as massive as Earth MJ 3 1782838 102M displaystyle M mathrm J 3 1782838 times 10 2 M oplus Context and implicationsJupiter s mass is 2 5 times that of all the other planets in the Solar System combined this is so massive that its barycenter with the Sun lies beyond the Sun s surface at 1 068 solar radii from the Sun s center Because the mass of Jupiter is so large compared to the other objects in the Solar System the effects of its gravity must be included when calculating satellite trajectories and the precise orbits of other bodies in the Solar System including the Moon and even Pluto Theoretical models indicate that if Jupiter had much more mass than it does at present its atmosphere would collapse and the planet would shrink For small changes in mass the radius would not change appreciably but above about 500 ME 1 6 Jupiter masses the interior would become so much more compressed under the increased pressure that its volume would decrease despite the increasing amount of matter As a result Jupiter is thought to have about as large a diameter as a planet of its composition and evolutionary history can achieve The process of further shrinkage with increasing mass would continue until appreciable stellar ignition was achieved as in high mass brown dwarfs having around 50 Jupiter masses Jupiter would need to be about 80 times as massive to fuse hydrogen and become a star Gravitational constantThe mass of Jupiter is derived from the measured value called the Jovian mass parameter which is denoted with GMJ The mass of Jupiter is calculated by dividing GMJ by the constant G For celestial bodies such as Jupiter Earth and the Sun the value of the GM product is known to many orders of magnitude more precisely than either factor independently The limited precision available for G limits the uncertainty of the derived mass For this reason astronomers often prefer to refer to the gravitational parameter rather than the explicit mass The GM products are used when computing the ratio of Jupiter mass relative to other objects In 2015 the International Astronomical Union defined the nominal Jovian mass parameter to remain constant regardless of subsequent improvements in measurement precision of MJ This constant is defined as exactly GM JN 1 2668653 1017 m3 s2 displaystyle mathcal GM mathrm J mathrm N 1 266 8653 times 10 17 text m 3 text s 2 If the explicit mass of Jupiter is needed in SI units it can be calculated by dividing GM by G where G is the gravitational constant Mass compositionThe majority of Jupiter s mass is hydrogen and helium These two elements make up more than 87 of the total mass of Jupiter The total mass of heavy elements other than hydrogen and helium in the planet is between 11 and 45 ME The bulk of the hydrogen on Jupiter is solid hydrogen Evidence suggests that Jupiter contains a central dense core If so the mass of the core is predicted to be no larger than about 12 ME The exact mass of the core is uncertain due to the relatively poor knowledge of the behavior of solid hydrogen at very high pressures Relative massMasses of noteworthy astronomical objects relative to the mass of Jupiter Object MJ Mobject Mobject MJ Ref Sun 9 547919 15 10 4 1047 348644 17 Earth 317 82838 0 003146 3520Jupiter 1 1 by definitionSaturn 3 3397683 0 299421 97Uranus 21 867552 0 045729 856Neptune 18 53467 0 053952 95Gliese 229B 21 52 451 Pegasi b 0 472 0 039See alsoJupiter radius Hot Jupiter Orders of magnitude mass Planetary mass Solar massNotesSome of the values in this table are nominal values derived from Numerical Standards for Fundamental Astronomy and rounded using appropriate attention to significant figures as recommended by the IAU Resolution B3 References Planets and Pluto Physical Characteristics ssd jpl nasa gov Jet Propulsion Labritory Retrieved 31 October 2017 Coffey Jerry 18 June 2008 Mass of Jupiter Universe Today Retrieved 2017 10 31 Numerical Standards for Fundamental Astronomy maia usno navy mil IAU Working Group Archived from the original on 26 August 2016 Retrieved 31 October 2017 MacDougal Douglas W November 6 2012 A Binary System Close to Home How the Moon and Earth Orbit Each Other Newton s Gravity Undergraduate Lecture Notes in Physics Springer New York pp 193 211 doi 10 1007 978 1 4614 5444 1 10 ISBN 9781461454434 the barycenter is 743 000 km from the center of the sun The Sun s radius is 696 000 km so it is 47 000 km above the surface Seager S Kuchner M Hier Majumder C A Militzer B 2007 Mass Radius Relationships for Solid Exoplanets The Astrophysical Journal 669 2 1279 1297 arXiv 0707 2895 Bibcode 2007ApJ 669 1279S doi 10 1086 521346 S2CID 8369390 How the Universe Works 3 Vol Jupiter Destroyer or Savior Discovery Channel 2014 Guillot Tristan 1999 Interiors of Giant Planets Inside and Outside the Solar System Science 286 5437 72 77 Bibcode 1999Sci 286 72G doi 10 1126 science 286 5437 72 PMID 10506563 Burrows Adam Hubbard William B Saumon D Lunine Jonathan I 1993 An expanded set of brown dwarf and very low mass star models Astrophysical Journal 406 1 158 71 Bibcode 1993ApJ 406 158B doi 10 1086 172427 Mamajek E E Prsa A Torres G et al 2015 IAU 2015 Resolution B3 on Recommended Nominal Conversion Constants for Selected Solar and Planetary Properties arXiv 1510 07674 astro ph SR Guillot Tristan Stevenson David J Hubbard William B Saumon Didier The Interior of Jupiter PDF Retrieved 31 October 2017 Guillot Tristan Gautier Daniel Hubbard William B December 1997 New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models Icarus 130 2 534 539 arXiv astro ph 9707210 Bibcode 1997Icar 130 534G doi 10 1006 icar 1997 5812 S2CID 5466469 Opik E J January 1962 Jupiter Chemical composition structure and origin of a giant planet Icarus 1 1 6 200 257 Bibcode 1962Icar 1 200O doi 10 1016 0019 1035 62 90022 2 Planetary Fact Sheet Ratio to Earth nssdc gsfc nasa gov Retrieved 2016 02 12 White Stephen M Jackson Peter D Kundu Mukul R December 1989 A VLA survey of nearby flare stars Astrophysical Journal Supplement Series 71 895 904 Bibcode 1989ApJS 71 895W doi 10 1086 191401 Martins J H C Santos N C Figueira P et al 2015 Evidence for a spectroscopic direct detection of reflected light from 51 Peg b Astronomy amp Astrophysics 576 2015 A134 arXiv 1504 05962 Bibcode 2015A amp A 576A 134M doi 10 1051 0004 6361 201425298 S2CID 119224213