{|style="width:100%;border-collapse:collapse;border:1px solid black;"
|+JUPITER'S SATELLITES.
|-
||No.
| colspan=4|Sidereal
Revolution.
||Distance.
Jupiter's
radius
= 1.
| colspan=3|Orbit
inclined to
Jupiter's
equator.
||Diameter
in miles.
||Mass.
Jupiter
=1
| colspan=2|Apparent
Diameter
from
Jupiter.
|-
||
||d.
||h.
||m.
||s.
||
||°
||′
||″
||
||
||′
||″
|-
||1|||1|||18|||27|||23|||6.048|||0|||0|||7|||2436|||.000017|||31|||11
|-
||2|||3|||13|||13|||42|||9.623|||0|||1|||6|||2187|||.000023|||17|||35
|-
||3|||7|||3|||42|||33|||15.350|||0|||5|||3|||3573|||.000088|||18|||0
|-
||4|||16|||16|||32|||11|||26.998|||0|||0|||24|||3057|||.000043|||8|||46
|}
|
[1] (Mean longitude of the 1st + twice mean longitude of 3d) 3 times mean longitude of 2d is always = , |
180° |
- ↑ In consequence of this remarkable relation, the 1st, 2d, and 3d satellites can never be eclipsed all at once.
| Volume (Earth's = 1), | 772 |
| Mass (Earth's = 1), . | 101.364 |
| Density (Earth's = 1), | .131 |
| Diameter (Earth's = 1), | 9.022 |
| in miles, | 75.070 |
| apparent, mean, | 17″.1 |
| minimum. | 15″.0 |
| maximum. | 20″.0 |
| Gravity (Earth's = 1), | 1.09 |
| bodies fall in one second, in feet, | 17.6 |
| Light and heat from Sun, perihelion (Earth's = 1) | .0123 |
| aphelion, | .0099 |
| mean, | .0111 |
| Polar less than equatorial diameter. | 1-10th |
| Distance from the Sun, mean, in miles, | 906,205,000 |
| , (Earth's = 1), | 9,538,850 |
| maximum, | 10,073,270 |
| minimum, | 9,004,422 |
| Eccentricity of orbit (semi-axis major = 1), | .0560265 |