

Unlike most planets, but similar to Uranus, Pluto rotates
with its poles almost in its orbital plane. Pluto's rotational axis is tipped
122 degrees. When Pluto was first discovered, its relatively bright south polar
region was the view seen from the Earth. Pluto appeared to grow dim as our
viewpoint gradually shifted from nearly pole-on in 1954 to nearly equator-on in
1973. Pluto's equator is now the view seen from Earth. During the period from
1985 through 1990, Earth was aligned with the orbit of Charon around Pluto such
that an eclipse could be observed every Pluto day. This provided opportunity to
collect significant data which led to albedo maps defining surface reflectivity,
and to the first accurate determination of the sizes of Pluto and Charon,
including all the numbers that could be calculated therefrom. The first eclipses
(mutual events) began blocking the north polar region. Later eclipses blocked
the equatorial region, and final eclipses blocked Pluto's south polar region. By
carefully measuring the brightness over time, it was possible to determine
surface features. It was found that Pluto has a highly reflective south polar
cap, a dimmer north polar cap, and both bright and dark features in the
equatorial region. Pluto's geometric albedo is 0.49 to 0.66, which is much
brighter than Charon. Charon's albedo ranges from 0.36 to 0.39. The eclipses
lasted as much as four hours and by carefully timing their beginning and ending,
measurements for their diameters were taken. The diameters can also be measured
directly to within about 1 percent by more recent images provided by the Hubble
Space Telescope. These images resolve the objects to clearly show two separate
disks. The improved optics allow us to measure Pluto's diameter as 2,274
kilometers (1413 miles) and Charon's diameter as 1,172 kilometers (728 miles),
just over half the size of Pluto. Their average separation is 19,640 km (12,200
miles). That's roughly eight Pluto diameters. Average separation and orbital
period are used to calculate Pluto and Charon's masses. Pluto's mass is about
6.4 x 10-9 solar masses. This is close to 7 (was 12 x's) times the
mass of Charon and approximately 0.0021 Earth mass, or a fifth of our moon.

Pluto's average density lies between 1.8 and 2.1 grams per cubic centimeter. It is concluded that Pluto is 50% to 75% rock mixed with ices. Charon's density is 1.2 to 1.3 g/cm3, indicating it contains little rock. The differences in density tell us that Pluto and Charon formed independently, although Charon's numbers derived from HST data are still being challenged by ground based observations. Pluto and Charon's origin remains in the realm of theory. Pluto's icy surface is 98% nitrogen (N2). Methane (CH4) and traces of carbon monoxide (CO) are also present. The solid methane indicates that Pluto is colder than 70 Kelvin. Pluto's temperature varies widely during the course of its orbit since Pluto can be as close to the sun as 30 AU and as far away as 50 AU. There is a thin atmosphere that freezes and falls to the surface as the planet moves away from the Sun. NASA plans to launch a spacecraft, the Pluto Express, in 2001 that will allow scientists to study the planet before its atmosphere freezes. The atmospheric pressure deduced for Pluto's surface is 1/100,000 that of Earth's surface pressure.