From: Classes of the solar wind interactions in the solar system
Object | B, nT | M, kg | Comment on neutral gas mass |
---|---|---|---|
Global interactions | Â | Â | Â |
Mercury | 195 | 6.6 103 | N = 4.4 104 O/cm−3 (Wurz and Lammer, 2003) |
Venus | 10 | 4.8 1020 | Â |
Earth | 3.08 104 | 5.3 1018 | Â |
Moon | 7 | 2.7 104 | Â |
Mars | 3.4 | 2.5 1016 | Â |
Ancient Mars | 60 | 2.0 1018 | 0.5 bar surface pressure |
Phobos | 3.4 | 2.7 103 | Q = 1023 s−1 (upper limit, Ip and Banaszkiewicz, 1990) |
Jupiter | 4.25 105 | 2.6 1020 | M from 1 bar level |
Ganymede | 770 | 1.8 105 | Â |
Callisto | 23 | 1.2 107 | Â |
Saturn | 2.0 104 | 4.3 1020 | M from 1 bar level |
Titan | 5 | 9.0 1018 | Â |
Uranus | 2.3 104 | 9.5 1019 | M from 1 bar level |
Neptune | 1.4 104 | 6.9 1019 | M from 1 bar level |
Comet Hale-Bopp | 7 | 2.7 1011 | Q = 1.0 1031 s−1 (Biver et al., 1997) |
Comet 26P/Grigg-Skjellerup | 7 | 1.3 108 | Q = 7.5 1027 s−1 (Johnstone et al., 1993) |
Small scale interactions | Â | Â | Â |
Lunar magnetic anomalies | 300 | 2.7 104 | M same as for the Moon |
Mars magnetic anomalies | 1500 | 2.5 1016 | M same as for Mars |