|
|
Natural Satellites Data Center. Parameters and constants
Satellites of Mars
Satellites of Jupiter
Satellites of Saturn
Satellites of Uranus
Satellites of Neptune
Satellites of Pluto
|
Satellites of Jupiter
|
Gm [km3/s2]
|
References
|
Sources of the data
|
|
J1 Io
|
5961±10
5959.92±0.02
|
Campbell J.K., Synnott S.P., 1985
Jacobson R. A., 2001
|
Voyager tracking data
Galileo mission
|
|
J2 Europa
|
3201±10
3202.73±0.02
|
Campbell J.K., Synnott S.P., 1985
Jacobson R. A., 2001
|
Voyager tracking data
Galileo mission
|
|
J3 Ganymede
|
9887±3
9887.83±0.03
|
Campbell J.K., Synnott S.P., 1985
Jacobson R. A., 2001
|
Voyager tracking data
Galileo mission
|
|
J4 Callisto
|
7181±3
7179.29±0.02
|
Campbell J.K., Synnott S.P., 1985
Jacobson R. A., 2001
|
Voyager tracking data
Galileo mission Doppler tracking
|
|
J5 Amalthea
|
0.139±0.010
|
Anderson et al. 2005
|
Galileo Radio Doppler data
|
|
J6 Himalia
|
0.45
0.28±0.04
|
Rettig, Walsh, 2002
Emelyanov N.V., 2005
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
Perturbations on other satell.
|
|
J7 Elara
|
0.058
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J8 Pasiphae
|
0.020
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J9 Sinope
|
0.0050
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J10 Lysithea
|
0.0042
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J11 Carme
|
0.0088
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J12 Ananke
|
0.0020
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J13 Leda
|
0.00073
|
Rettig, Walsh, 2002
|
Photometric observations
with the density of 2.6 g/cm3
and the albedo of 0.04
(assumed)
|
|
J14 Tebe
|
0.10
|
Thomas et al. 1998
|
Images made by "Galileo"
with the density assumed of 3.0 g/cm3
|
|
J15 Adrastea
|
0.0005
|
Thomas et al. 1998
|
Images made by "Galileo"
with the density assumed of 3.0 g/cm3
|
|
J16 Metis
|
0.008
|
Thomas et al. 1998
|
Images made by "Galileo"
with the density assumed of 3.0 g/cm3
|
Estimations made on the basis of reduction
of the photometric data published in the MPC (Emel'yanov, Ural'skaya, 2011, Solar System Research, 45, 377)
( See photometric parameters of sateliites in this database)
using the equations
(Bowell et al., 1989))
log pH=6.114-2 log(2r )-0.4 H , Gm=G 4/3 π r3 ρ
where r - radius of satellite,
H - absolute magnitude in R band at solar distance 1 au, observer distance 1 au,
reduced at phase angle α=0°, pH - assumed albedo
in R band,
ρ - assumed density of satellite [g/cm3].
|
Satellites of Jupiter
|
Gm [km3/s2]
|
Source of the data
|
| J17 Callirrhoe | 0.0000672 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J18 Themisto | 0.0000442 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J19 Megaclite | 0.0000270 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J20 Taygete | 0.0000145 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J21 Chaldene | 0.0000095 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J22 Harpalyke | 0.0000106 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J23 Kalyke | 0.0000196 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J24 Iocaste | 0.0000177 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J25 Erinome | 0.0000048 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J26 Isonoe | 0.0000078 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J27 Praxidike | 0.0000361 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J28 Autonoe | 0.0000099 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J29 Thyone | 0.0000088 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J30 Hermippe | 0.0000189 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J31 Aitne | 0.0000051 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J32 Eurydome | 0.0000054 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J33 Euanthe | 0.0000055 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J34 Euporie | 0.0000031 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J35 Orthosie | 0.0000042 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J36 Sponde | 0.0000035 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J37 Kale | 0.0000031 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J38 Pasithee | 0.0000021 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J39 Hegemone | 0.0000043 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J40 Mneme | 0.0000042 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J41 Aoede | 0.0000082 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J42 Thelxinoe | 0.0000044 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J43 Arche | 0.0000036 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J44 Kallichore | 0.0000029 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J45 Helike | 0.0000091 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J46 Carpo | 0.0000043 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J47 Eukelade | 0.0000090 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J48 Cyllene | 0.0000030 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J49 Kore | 0.0000050 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| J50 Herse | 0.0000032 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 2 | 0.0000019 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 3 | 0.0000016 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 4 | 0.0000012 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 5 | 0.0000124 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 9 | 0.0000012 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 10 | 0.0000012 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 12 | 0.0000008 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 15 | 0.0000017 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 16 | 0.0000017 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 18 | 0.0000037 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 19 | 0.0000016 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2003 J 23 | 0.0000012 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2010 J 1 | 0.0000025 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2010 J 2 | 0.0000007 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2011 J 1 | 0.0000012 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2011 J 2 | 0.0000012 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2016 J 1 | 0.0000035 | Photometry, assumed albedo of 0.04 and density of 2.6 |
| S/2017 J 1 | 0.0000091 | Photometry, assumed albedo of 0.04 and density of 2.6 |
Satellites of Saturn
See also the next table
|
Gm [km3/s2]
|
References
|
Sources of the data (EB - Earth-based,
HST - Hubble Space Telescope observations)
|
|
S1 Mimas
|
2.5023±0.0020
2.504±0.002
2.509±0.004
|
Jacobson R.A. et al., 2006
Jacobson R.A. et al., 2006a
Cooper et al., 2008
|
EB, Pioneer 11, Voyager, and Cassini data
|
|
S2 Enceladus
|
7.2096±0.0067
7.205±0.011
|
Jacobson R.A. et al., 2006
Rappaport N. et al., 2007
|
EB, Pioneer 11, Voyager, and Cassini data
Doppler data of the Cassini
|
|
S3 Tethys
|
41.2097±0.0063
41.200±0.007
|
Jacobson R.A. et al., 2006
Jacobson R.A. et al., 2006a
|
EB, Pioneer 11, Voyager, and Cassini data
|
|
S4 Dione
|
73.1127±0.0025
|
Jacobson R.A. et al., 2006
|
EB, Pioneer 11, Voyager, and Cassini data
|
|
S5 Rhea
|
153.9416±0.0049
153.9395±0.0018
|
Jacobson R.A. et al., 2006
Iess L. et al., 2007
|
EB, Pioneer 11, Voyager, and Cassini data
Cassini Doppler data
|
|
S6 Titan
|
8978.1356±0.0039
8978.1394
|
Jacobson R.A. et al., 2006
Iess et al., 2010
|
EB, Pioneer 11, Voyager, and Cassini data
Radio tracking of the spacecraft Cassini
|
|
S7 Hyperion
|
0.3727±0.0045
|
Jacobson R.A. et al., 2006
|
EB, Pioneer 11, Voyager, and Cassini data
|
|
S8 Iapetus
|
120.20±0.06
120.5117±0.0173
|
Rappaport et al., 2005
Jacobson R.A. et al., 2006
|
Cassini gravity experiments
EB, Pioneer 11, Voyager, and Cassini data
|
|
S9 Phoebe
|
0.5517±0.0007
0.5534±0.0006
|
Rappaport et al., 2005
Jacobson R.A. et al., 2006
|
Cassini gravity experiments
EB, Pioneer 11, Voyager, and Cassini data
|
|
S10 Janus
|
0.1266±0.00008
0.12651±0.00003
0.126403±0.000019
|
Jacobson et al., 2008
Cooper et al., 2015
Lainey et al., 2023
|
Mutual perturbations of satelltes (Cassini)
New Cassini Imaging
Cassini-Huygens space mission
|
|
S11 Epimetheus
|
0.03513±0.00002
0.035110±0.000009
0.0350806±0.0000054
|
Jacobson et al., 2008
Cooper et al., 2015
Lainey et al., 2023
|
Mutual perturbations of satelltes (Cassini)
New Cassini Imaging
Cassini-Huygens space mission
|
|
S12 Helene
|
0.0017
|
Thomas P. C., 1989
|
Images made by "Voyager"
with the density of 1.5 g/cm3
and the albedo of 0.6
(assumed)
|
|
S13 Telesto
|
0.00048
|
Thomas et al., 1983
|
Images made by "Voyager"
with the density of 1.0 g/cm3
and the albedo of 1.0
(assumed)
|
|
S14 Calypso
|
0.00024
|
Thomas et al., 1983
|
Images made by "Voyager"
with the density of 1.5 g/cm3
and the albedo of 0.7
(assumed)
|
|
S15 Atlas
|
0.000384±0.000001
0.000384±0.000001
0.0003664±0.0000028
|
Jacobson et al., 2008
Cooper et al., 2015
Lainey et al., 2023
|
Mutual perturbations of satelltes (Cassini)
New Cassini Imaging
Cassini-Huygens space mission
|
|
S16 Prometheus
|
0.0141±0.0025
0.01064±0.00010
0.010677±0.000006
|
Jacobson et al., 2008
Cooper et al., 2015
Lainey et al., 2023
|
Mutual perturbations of satelltes (Cassini)
New Cassini Imaging
Cassini-Huygens space mission
|
|
S17 Pandora
|
0.00915±0.00013
0.009133±0.000009
0.009058±0.000011
|
Jacobson et al., 2008
Cooper et al., 2015
Lainey et al., 2023
|
Mutual perturbations of satelltes (Cassini)
New Cassini Imaging
Cassini-Huygens space mission
|
|
S18 Pan
|
0.00033±0.00005
|
Porco et al., 2005
|
Mutual perturbations of satelltes (Cassini)
|
Estimations made on the basis of reduction
of the photometric data published in the MPC (Emel'yanov, Ural'skaya, 2011, Solar System Research, 45, 377)
( See photometric parameters of sateliites in this database)
using the equations
(Bowell et al., 1989))
log pH=6.114-2 log(2r )-0.4 H , Gm=G 4/3 π r3 ρ
where r - radius of satellite,
H - absolute magnitude in R band at solar distance 1 au, observer distance 1 au,
reduced at phase angle α=0°, pH - assumed albedo
in R band,
ρ - assumed density of satellite [g/cm3].
|
Satellites of Saturn
|
Gm [km3/s2]
|
Source of the data
|
| S19 Ymir | 0.0005264 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S20 Paaliaq | 0.0008621 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S21 Tarvos | 0.0002069 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S22 Ijiraq | 0.0001232 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S23 Suttungr | 0.0000160 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S24 Kiviuq | 0.0003273 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S25 Mundilfari | 0.0000176 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S26 Albiorix | 0.0016549 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S27 Skathi | 0.0000223 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S28 Erriapo | 0.0000870 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S29 Siarnaq | 0.0091789 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S30 Thrymr | 0.0000314 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S31 Narvi | 0.0000129 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S36 Aegir | 0.0000081 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S37 Bebhionn | 0.0000099 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S38 Bergelmir | 0.0000094 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S39 Bestla | 0.0000164 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S40 Farbauti | 0.0000043 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S41 Fenrir | 0.0000036 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S42 Fornjot | 0.0000080 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S43 Hati | 0.0000070 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S44 Hyrrokkin | 0.0000366 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S45 Kari | 0.0000155 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S46 Loge | 0.0000088 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S47 Skoll | 0.0000090 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S48 Surtur | 0.0000048 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S50 Jarnsaxa | 0.0000044 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S51 Greip | 0.0000060 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S52 Tarqeq | 0.0000146 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2004 S 7 | 0.0000076 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2004 S 12 | 0.0000054 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2004 S 13 | 0.0000056 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2004 S 17 | 0.0000031 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2006 S 1 | 0.0000073 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2006 S 3 | 0.0000038 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2007 S 2 | 0.0000094 | Photometry, assumed albedo of 0.06 and density of 2.3 |
| S/2007 S 3 | 0.0000045 | Photometry, assumed albedo of 0.06 and density of 2.3 |
|
Satellites of Uranus
|
Gm [km3/s2]
|
References
|
Sources of the data
|
|
U1 Ariel
|
83.5±1.4
|
Jacobson et al., 2014
|
New dynamical model and extended set of observations (Earth-based, HST, Voyager-2)
|
|
U2 Umbriel
|
85.1±1.9
|
Jacobson et al., 2014
|
New dynamical model and extended set of observations (Earth-based, HST, Voyager-2)
|
|
U3 Titania
|
226.9±4.1
|
Jacobson et al., 2014
|
New dynamical model and extended set of observations (Earth-based, HST, Voyager-2)
|
|
U4 Oberon
|
205.3±5.8
|
Jacobson et al., 2014
|
New dynamical model and extended set of observations (Earth-based, HST, Voyager-2)
|
|
U5 Miranda
|
4.3±0.2
|
Jacobson et al., 2014
|
New dynamical model and extended set of observations (Earth-based, HST, Voyager-2)
|
|
U6 Cordelia
|
0.0030
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U7 Ophelia
|
0.0036
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U8 Bianca
|
0.0062
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U9 Cressida
|
0.0229
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U10 Desdemona
|
0.0119
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U11 Juliet
|
0.0372
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U12 Portia
|
0.1122
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U13 Rosalind
|
0.0170
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U14 Belinda
|
0.0238
|
Karkoschka, 2001
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
|
U15 Puck
|
0.1931
|
Thomas et al., 1989
|
Reduced from the images made by Voyager
with the density of 1.3 g/cm3
(assumed)
|
Estimations made on the basis of reduction
of the photometric data published in the MPC (Emel'yanov, Ural'skaya, 2011, Solar System Research, 45, 377)
( See photometric parameters of sateliites in this database)
using the equations
(Bowell et al., 1989))
log pH=6.114-2 log(2r )-0.4 H , Gm=G 4/3 π r3 ρ
where r - radius of satellite,
H - absolute magnitude in R band at solar distance 1 au, observer distance 1 au,
reduced at phase angle α=0°, pH - assumed albedo
in R band,
ρ - assumed density of satellite [g/cm3].
|
Satellites of Uranus
|
Gm [km3/s2]
|
Source of the data
|
| U16 Caliban | 0.0471079 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U17 Sycorax | 0.2704545 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U18 Prospero | 0.0065508 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U19 Setebos | 0.0082507 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U20 Stephano | 0.0020243 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U21 Trinculo | 0.0003434 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U22 Francisco | 0.0003815 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U23 Margaret | 0.0003531 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| U24 Ferdinand | 0.0005064 | Photometry, assumed albedo of 0.04 and density of 1.5 |
|
Satellites of Neptune
|
Gm [km3/s2]
|
References
|
Sources of the data
(EB - Earth-based)
|
|
N1 Triton
|
427.598±1.9
|
Jacobson et al., 2009
|
Earth based, HST, Voyager-2
|
|
N2 Nereid
|
2.06
|
Thomas et al., 1991
|
Images made by Voyager
with the density assumed of 1.5 g/cm3
|
|
N3 Naiad
|
0.013
|
Karkoschka E., 2003
|
Images made by Voyager
with the density assumed of 1.3 g/cm3
|
|
N4 Thalassa
|
0.025
|
Karkoschka E., 2003
|
Images made by Voyager
with the density assumed of 1.3 g/cm3
|
|
N5 Despina
|
0.14
|
Karkoschka E., 2003
|
Images made by Voyager
with the density assumed of 1.3 g/cm3
|
|
N6 Galatea
|
0.25
|
Karkoschka E., 2003
|
Images made by Voyager
with the density assumed of 1.3 g/cm3
|
|
N7 Larissa
|
0.33
|
Karkoschka E., 2003
|
Images made by Voyager
with the density assumed of 1.3 g/cm3
|
|
N8 Proteus
|
3.36
|
Karkoschka E., 2003
|
Images made by Voyager
with the density assumed of 1.3 g/cm3
|
Estimations made on the basis of reduction
of the photometric data published in the MPC (Emel'yanov, Ural'skaya, 2011, Solar System Research, 45, 377)
( See photometric parameters of sateliites in this database)
using the equations
(Bowell et al., 1989))
log pH=6.114-2 log(2r )-0.4 H , Gm=G 4/3 π r3 ρ
where r - radius of satellite,
H - absolute magnitude in R band at solar distance 1 au, observer distance 1 au,
reduced at phase angle α=0°, pH - assumed albedo
in R band,
ρ - assumed density of satellite [g/cm3].
|
Satellites of Neptune
|
Gm [km3/s2]
|
Source of the data
|
| N9 Halimede | 0.0210759 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| N10 Psamathe | 0.0044054 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| N11 Sao | 0.0038316 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| N12 Laomedeia | 0.0063181 | Photometry, assumed albedo of 0.04 and density of 1.5 |
| N13 Neso | 0.0091746 | Photometry, assumed albedo of 0.04 and density of 1.5 |
|
Satellites of Pluto
|
Gm [km3/s2]
|
References
|
Sources of the data
|
|
System
|
975.5±1.5
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
Pluto
|
869.6±1.8
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
P1 Charon
|
105.9±1.0
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
P2 Nix
|
0.0030±0.0027
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
P3 Hydra
|
0.0032±0.0028
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
P4 Kerberos
|
0.0011±0.0006
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
P5 Styx
|
0.0010
|
Brozovic et al., 2015
|
Earth-based, HST, Mutual events
|
|
|