Although Pluto was discovered in 1930, limited information on the distant planet delayed a realistic understanding of
its characteristics. Today Pluto remains the only planet that has not been visited by a spacecraft, yet an increasing amount
of information is unfolding about this peculiar planet. The uniqueness of Pluto's orbit, rotational relationship with its
satellite, spin axis, and light variations all give the planet a certain appeal.
Pluto is usually farther from the Sun than any of the nine planets; however, due to the eccentricity of its orbit, it is closer than Neptune for 20 years out of its 249 year orbit. Pluto crossed Neptune's orbit January 21, 1979, made its closest approach September
5, 1989, and will remain within the orbit of Neptune until February 11, 1999. This will not occur again until September 2226.
As Pluto approaches perihelion it reaches its maximum distance from the ecliptic due to its 17-degree inclination. Thus, it is far above or below the plane of Neptune's orbit. Under these conditions, Pluto
and Neptune will not collide and do not approach closer than 18 A.U. to one another.
Pluto's rotation period is 6.387 days, the same as its satellite Charon. Although it is common for a satellite to travel
in a synchronous orbit with its planet, Pluto is the only planet to rotate synchronously with the orbit of its satellite. Thus being tidally locked,
Pluto and Charon continuously face each other as they travel through space.
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
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.
Pluto was officially labeled the ninth planet by the International Astronomical Union in 1930 and named for the Roman god
of the underworld. It was the first and only planet to be discovered by an American, Clyde W. Tombaugh.
The path toward its discovery is credited to Percival Lowell who founded the Lowell Observatory in Flagstaff, Arizona and
funded three separate searches for "Planet X." Lowell made numerous unsuccessful calculations to find it, believing it could
be detected from the effect it would have on Neptune's orbit. Dr. Vesto Slipher, the observatory director, hired Clyde Tombaugh
for the third search and Clyde took sets of photographs of the plane of the solar system (ecliptic) one to two weeks apart
and looked for anything that shifted against the backdrop of stars. This systematic approach was successful and Pluto was
discovered by this young (born 4 Feb 1906) 24 year old Kansas lab assistant on February 18, 1930. Pluto is actually too small
to be the "Planet X" Percival Lowell had hoped to find. Pluto's was a serendipitous discovery.
||Clyde W. Tombaugh|
|Date of discovery
||February 18, 1930|
|Mass (Earth = 1)
|Equatorial radius (km)
|Equatorial radius (Earth = 1)
|Mean density (gm/cm^3)
|Mean distance from the Sun (km)
|Mean distance from the Sun (Earth = 1))
|Rotational period (days)
|Orbital period (years)
|Mean orbital velocity (km/sec)
|Tilt of axis (degrees)
|Orbital inclination (degrees)
|Equatorial surface gravity (m/sec^2)
|Equatorial escape velocity (km/sec)
|Visual geometric albedo
Pluto & Charon
This view of Pluto was taken by the Hubble Space Telescope. It shows a rare image of tiny Pluto
with its moon Charon, which is slightly smaller than the planet. Because Pluto has not yet been visited by any spacecraft,
it remains a mysterious planet. Due to its great distance from the sun, Pluto's surface is believed to reach temperatures
as low as -240°C (-400°F). From Pluto's surface, the Sun appears as only a very bright star. (Courtesy NASA)
Hubble Telescope Image
This is the clearest view yet of the distant planet Pluto and its moon, Charon, as revealed
by the Hubble Space Telescope (HST). The image was taken on February 21, 1994, when the planet was 4.4 billion kilometers
(2.7 billion miles) from the Earth.
The HST corrected optics show the two objects as clearly separate and sharp disks. This now allows astronomers to measure
directly (to within about 1 percent) Pluto's diameter of 2,320 kilometers (1,440 miles) and Charon's diameter of 1,270 kilometers
The HST observations show that Charon is bluer than Pluto. This means that the worlds have different surface composition
and structure. A bright highlight on Pluto indicates that it might have a smoothly reflecting surface layer. A detailed analysis
of the HST image also suggests that there is a bright area parallel to the equator of Pluto. However, subsequent observations
are needed to confirm that this feature is real. The new HST image was taken when Charon was near its maximum elongation from
Pluto (0.9 arcseconds). The two worlds are 19,640 kilometers (12,200 miles) apart. (Courtesy NASA/ESA/ESO)
The Surface of Pluto
The never-before-seen surface of the distant planet Pluto is resolved in these NASA Hubble
Space Telescope pictures. These images, which were made in blue light, show that Pluto is an unusually complex object, with
more large-scale contrast than any planet, except Earth. Pluto probably shows even more contrast and perhaps sharper boundaries
between light and dark areas than is shown here, but Hubble's resolution (just like early telescopic views of Mars) tends
to blur edges and blend together small features sitting inside larger ones.
The two smaller inset pictures at the top are actual images from Hubble. North is up. Each square pixel (picture element)
is more than 100 miles across. At this resolution, Hubble discerns roughly 12 major "regions" where the surface is either
bright or dark. The larger images (bottom) are from a global map constructed through computer image processing performed on
the Hubble data. Opposite hemispheres of Pluto are seen in these two views. (Courtesy NASA/ESA/ESO)
Pluto, Charon, and USA Comparison
This image shows the approximate size of Pluto and Charon by overlaying them
on an Advanced Very High Resolution Radiometer (AVHRR) image of the United States of America. Pluto is about 2274 kilometers
(1410 miles) in diameter and Charon 1172 kilometers (727 miles) in diameter. The image of Pluto is based upon Hubble observations
taken of Pluto in June and July of 1994. The Charon image is based upon photometric measurements acquired by Marc Buie of
Lowell Observatory. (Copyright 1998 by Calvin J. Hamilton)
Map of the Surface of Pluto
This is the first image-based surface map of the solar system's most remote planet,
Pluto. The map, which covers 85% of the planet's surface, confirms that Pluto has a dark equatorial belt and bright polar
caps, as inferred from ground-based light curves obtained during the mutual eclipses that occurred between Pluto and its satellite
Charon in the late 1980s.
The brightness variations in this map may be due to topographic features such as basins and fresh impact craters. However,
most of the surface features are likely produced by the complex distribution of frosts that migrate across Pluto's surface
with its orbital and seasonal cycles and chemical byproducts deposited out of Pluto's nitrogen-methane atmosphere. Names may
later be proposed for some of the larger regions.
Image reconstruction techniques smooth out the coarse pixels in the four raw images to reveal major regions where the surface
is either bright or dark. The black strip across the bottom corresponds to the region surrounding Pluto's south pole, which
was pointed away from Earth when the observations were made, and could not be imaged. (Courtesy NASA/ESA/ESO)
Ground vs. Hubble Comparison
This image shows a comparison between a ground based view (left) and a Hubble Space
Telescope view (right) of Pluto and Charon.
Nordic Optical Telescope
This image of Pluto was taken with the 2.6 meter Nordic Optical Telescope, located at La Palma, Canary Islands. It is a good example of the best imagery that can be obtained from Earth-based telescopes.
(© Copyright Nordic Optical Telescope Scientific Association -- NOTSA)
This is a painting by Pat Rawlings of the Pluto Express mission scheduled for launch in 2001 to
arrive at Pluto around 2006-2008. The mission will consist of a pair of small, fast, relatively cheap spacecraft weighing
less than 100 kilograms (220 pounds) each. The spacecraft will pass within 15,000 kilometers (9,300 miles) of Pluto and Charon.
(Courtesy Pat Rawlings/NASA/JPL)