SYNOPTICAL TABLES.
347
{|style="width:100%;border-collapse:collapse;border:1px solid black;"
|+JUPITER'S SATELLITES.
|-style="font-size:83%;text-align:center;vertical-align:middle;border-bottom:1px solid black;"
|style="border-right:1px solid black;"|No.
|style="border-right:1px solid black;" colspan=4|Sidereal
Revolution.
|style="border-right:1px solid black;"|Distance.
Jupiter's
radius
= 1.
|style="border-right:1px solid black;" colspan=3|Orbit
inclined to
Jupiter's
equator.
|style="border-right:1px solid black;"|Diameter
in miles.
|style="border-right:1px solid black;"|Mass.
Jupiter
=1
|style="border-right:1px solid black;" colspan=2|Apparent
Diameter
from
Jupiter.
|-
|style="border-right:1px solid black;"|
|style="text-align:center;"|d.
|style="text-align:center;"|h.
|style="text-align:center;"|m.
|style="text-align:center;border-right:1px solid black;"|s.
|style="border-right:1px solid black;"|
|style="text-align:center;"|°
|style="text-align:center;"|′
|style="text-align:center;border-right:1px solid black;"|″
|style="border-right:1px solid black;"|
|style="border-right:1px solid black;"|
|style="text-align:center;"|′
|style="text-align:center;border-right:1px solid black;"|″
|-
|style="text-align:right;border-right:1px solid black;"|1||style="text-align:right;"|1||style="text-align:right;"|18||style="text-align:right;"|27||style="text-align:right;border-right:1px solid black;"|23||style="text-align:right;border-right:1px solid black;"|6.048||style="text-align:right;"|0||style="text-align:right;"|0||style="text-align:right;border-right:1px solid black;"|7||style="text-align:right;border-right:1px solid black;"|2436||style="text-align:right;border-right:1px solid black;"|.000017||style="text-align:right;"|31||style="text-align:right;"|11
|-
|style="text-align:right;border-right:1px solid black;"|2||style="text-align:right;"|3||style="text-align:right;"|13||style="text-align:right;"|13||style="text-align:right;border-right:1px solid black;"|42||style="text-align:right;border-right:1px solid black;"|9.623||style="text-align:right;"|0||style="text-align:right;"|1||style="text-align:right;border-right:1px solid black;"|6||style="text-align:right;border-right:1px solid black;"|2187||style="text-align:right;border-right:1px solid black;"|.000023||style="text-align:right;"|17||style="text-align:right;"|35
|-
|style="text-align:right;border-right:1px solid black;"|3||style="text-align:right;"|7||style="text-align:right;"|3||style="text-align:right;"|42||style="text-align:right;border-right:1px solid black;"|33||style="text-align:right;border-right:1px solid black;"|15.350||style="text-align:right;"|0||style="text-align:right;"|5||style="text-align:right;border-right:1px solid black;"|3||style="text-align:right;border-right:1px solid black;"|3573||style="text-align:right;border-right:1px solid black;"|.000088||style="text-align:right;"|18||style="text-align:right;"|0
|-
|style="text-align:right;border-right:1px solid black;"|4||style="text-align:right;"|16||style="text-align:right;"|16||style="text-align:right;"|32||style="text-align:right;border-right:1px solid black;"|11||style="text-align:right;border-right:1px solid black;"|26.998||style="text-align:right;"|0||style="text-align:right;"|0||style="text-align:right;border-right:1px solid black;"|24||style="text-align:right;border-right:1px solid black;"|3057||style="text-align:right;border-right:1px solid black;"|.000043||style="text-align:right;"|8||style="text-align:right;"|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 |
Diameter in miles, | 75.070 |
Diameter apparent, mean, | 17″.1 |
Diameter apparent minimum. | 15″.0 |
Diameter apparent maximum. | 20″.0 |
Gravity (Earth's = 1), | 1.09 |
Gravity bodies fall in one second, in feet, | 17.6 |
Light and heat from Sun, perihelion (Earth's = 1) | .0123 |
Light and heat from Sun aphelion, | .0099 |
Light and heat from Sun mean, | .0111 |
Polar less than equatorial diameter. | 1-10th |
Distance from the Sun, mean, in miles, | 906,205,000 |
Distance from the Sun, (Earth's = 1), | 9,538,850 |
Distance from the Sun, in miles, maximum, | 10,073,270 |
Distance from the Sun, in miles, minimum, | 9,004,422 |
Eccentricity of orbit (semi-axis major = 1), | .0560265 |