Encyclopedia of the Solar System 2nd ed

(Marvins-Underground-K-12) #1
488 Encyclopedia of the Solar System

FIGURE 6 Triton approach
sequence, overlaid with a
latitude-longitude grid. Details on
Triton’s surface unfold dramatically
as the resolution changes from
about 60 km/pixel at a distance of 5
million km for the image in the
upper left to about 5 km/pixel at a
distance of 0.5 million km for the
image in the lower right. Mainly
looking at the southern
hemisphere, Triton rotates
retrograde (counterclockwise) over
an observational period of 4.3 days.
(Courtesy of Alfred McEwen,
University of Arizona.)

indicates a prolonged history of melting and separation of
icy phases. In the model, ice, structurally represented by the
most abundant solar system ice (H 2 O) forms a deep mantle
around a rock+metal core. A metallic (Fe, Ni, and proba-
bly S) inner core is also shown. The proportions of rock and
metal in the core are fixed to solar composition (carbona-
ceous chondrite) values, because relatively involatile rock
and metal should have been completely condensed in the


TABLE 1 Properties of Triton

Radius,R 1352.5 km
Mass,M 2.140× 1022 kg
Surface gravity,g 0.78 m sec–^2
Mean density,ρ 2065 kg m–^3
Percent rock+metal by
mass

65–70%

Distance from Neptune 354.8× 103 km=14.33 RN
Distance from Sun 30.058 AU
Orbit Period 5.877 days
Orbit Period around Sun 164.8 yr
Eccentricity 0.0000(16)
Inclination (present) 156.8◦
Geometric albedo (average) 0.70
Bond Albedo (average) 0.85
Surface Temperature 38 K (1989), 39 K (2003)
Surface Composition N 2 ,H 2 O, CO 2 , CO, CH 4 ,
C 2 H 6 ices
Surface Atmospheric
Pressure

14 μbar (1989), 19μbar
(2003)
Atmospheric Composition N 2 , minor CH 4
Tropopause Height 8 km

outer solar system. Melting and separation of metal from
rock are justified by theoretical arguments for intense tidal
heating in Triton’s past, and by the example of Ganymede,
where theGalileoorbiter’s discovery of a dipole magnetic
field demands that such an inner metallic core exists.
Whether Triton is also a magnetized body depends on
when its tidal heating ended, butVoyager 2passed too far
away to tell. Triton is, however, a sufficiently rock-rich body
that solid-state convection in its icy mantle should be oc-
curring today, powered by the heat released by the decay of
U, Th, and^40 K in its rocky core. Its icy mantle should also
be warm enough to mobilize lower-melting-point ices such

FIGURE 7 Internal structure model for present-day Triton.
Free download pdf