This large debris disk is similar to the Kuiper Belt, which encircles the solar system and contains a range of icy bodies from dust grains to objects the size
of dwarf planets, such as Pluto.
When it was first discovered, Eris was thought to be the largest
of the dwarf planets, with a mass 27 percent larger than that of Pluto and a diameter of approximately 1,400 to 1,500 miles (2,300 to 2,400 km).
Pluto is the most well known
of the dwarf planets.
Ceres is the earliest known and smallest of the current category
of dwarf planets.
From the discovery of moons around these icy bodies, the internal composition, mass, density, and internal structure
of these dwarf planets has been revealed.
* Number of Stars: 1 (Our Sun) * Number of Planets: 8 * Number
of Dwarf Planets: 5 * Number of Comets: Over 3000 * Number of Asteroids: Over 550,000.
2015 is the year
of the dwarf planets.
The vast majority
of dwarf planets like RR245 were destroyed or thrown from the solar system as the giant planets moved out to their present positions.
Pluto and Charon make sense only if hundreds or thousands
of dwarf planets once roamed the outer solar system.
This image is
of the dwarf planet Ceres, in an asteroid belt between Mars and Jupiter, and the two points of light emanating from it have scientists puzzled.
Early images taken by New Horizons
of the dwarf planet's surface mean we have to rethink how the planet was formed
«This deployment of technical means allowed us to reconstruct with a very high precision the shape and size
of dwarf planet Haumea, and discover to our surprise that it is considerably bigger and less reflecting than was previously believed.
According to the data obtained from the stellar occultation, the ring lies on the equatorial plane
of the dwarf planet, just like its biggest satellite, Hi'iaka, and it displays a 3:1 resonance with respect to the rotation of Haumea, which means that the frozen particles which compose the ring rotate three times slower around the planet than it rotates around its own axis.
The ring is at a distance of 2287 kilometers from the center of the main body and is darker than the surface
of the dwarf planet itself.
THE shattered remnants
of a dwarf planet may have bombarded the inner planets in the early solar system, suggests a new analysis of craters on the moon.
THE half - digested remains
of a dwarf planet could provide the best insight yet into the chemical make - up of alien solar systems.
«New images
of dwarf planet Ceres.»
«Dawn snaps its best - yet image
of dwarf planet Ceres.»
But a model of Ceres presented at the LPSC has added a wrinkle by suggesting comet - like behaviour is only possible at the poles
of the dwarf planet, not the lower - latitude areas where the bright spot has been seen.
This image was taken by NASA's Dawn spacecraft
of dwarf planet Ceres on Feb. 19 from a distance of nearly 29,000 miles (46,000 kilometers).
In keeping with all the rest of Ceres's oddball uncertainties, the findings hold major albeit nebulous implications for our understanding
of the dwarf planet and its relationship to the other large objects in our solar system.
Weight from massive deposits of frozen nitrogen, methane and carbon monoxide, built up billions of years ago, could have carved out the left half
of the dwarf planet's heart - shaped landscape, researchers report online November 30 in Nature.
As a worldwide audience awaits images from NASA's New Horizons spacecraft flyby of Pluto on July 14, NAU scientists already are supporting astronomers» understanding
of the dwarf planet's surface.
If you could fly aboard NASA's Dawn spacecraft, the surface
of dwarf planet Ceres would generally look quite dark, but with notable exceptions.
Outflow of water vapour has been detected from the surface
of the dwarf planet Ceres, which is in the asteroid belt between Mars and Jupiter.
New Horizons» flyby
of the dwarf planet and its five known moons is providing an up - close introduction to the solar system's Kuiper Belt, an outer region populated by icy objects ranging in size from boulders to dwarf planets.
For example, they revealed that the west side of Pluto's «heart» is rich in carbon - monoxide ice, unlike the rest
of the dwarf planet, and they announced that the probe had detected Pluto's thin, nitrogen - dominated atmosphere out to a distance of 1,000 miles (1,600 km) from the surface.
This enhanced color image
of the dwarf planet helps scientists detect differences in the composition and texture of Pluto's surface.
This animation
of the dwarf planet Ceres was made by combining images taken by the Dawn spacecraft on January 25, 2015.
Last July, NASA's New Horizons spacecraft swooped near Pluto, snapping the first close - ups ever taken
of the dwarf planet's surface.
Mike Brown of the California Institute of Technology in Pasadena, whose discovery
of dwarf planet Eris led to Pluto's demotion, is upbeat: «Even objects that are not planets are interesting and have things about them yet to be discovered.»
A stunning image
of the dwarf planet in silhouette, released July 24, reveals a layer of haze extending...
The Hubble Space Telescope has provided the clearest images yet
of this dwarf planet for scientists to study.
Almost three years after NASA's New Horizons deep space probe made its historic flyby of Pluto, the International Astronomical Union (IAU) has released the first list of official names for features on the face
of the dwarf planet's largest moon, Charon.
Another view, showing an area in the southern mid-latitudes
of the dwarf planet.
These views
of dwarf planet Ceres were taken on 19 February from a distance of about 46,000 kilometres (29,000 miles) by NASA's Dawn spacecraft.
Some of the dwarf planet's features were named after mythologies around the world.
Dawn will also measure the gravity field of Ceres, which will provide more clues to the internal structure
of the dwarf planet.
The images will continue to improve as the spacecraft spirals closer to the surface during its 16 - month study
of the dwarf planet.
Over the next several weeks, Dawn will deliver increasingly better and better images
of the dwarf planet, leading up to the spacecraft's capture into orbit around Ceres on March 6.
Pluto may have recently been demoted to the status
of dwarf planet, but as astronomers learn more about this distant body, they are learning it behaves more like a planet than once believed.
A portion
of the dwarf planet Pluto's highly eccentric orbit brings it nearer to the Sun than Neptune, which has a nearly circular orbit.
Scientists hope further analysis
of the dwarf planet will reveal the true nature of the mystery lights.
NASA also unveiled new maps of Pluto and Charon last week to commemorate the spacecraft's July 14, 2015 flyby
of the dwarf planet and its satellites, which brought the probe to within 7,800 miles (12,550 kilometers) of Pluto's surface and allowed it to capture the first - ever up - close pics of the system — not to mention a considerable amount of game - changing scientific data.
If you're among the countless space science enthusiasts who wondered what the New Horizons spacecraft's 2015 flyover of Pluto might have looked like, you're in luck — NASA has released a new video that gives all of us an up - close look at the surface terrain
of the dwarf planet.
An artist's impression
of the dwarf planet Ceres, which appears to have a water vapor atmosphere from outgassing on the object.
NASA's Dawn spacecraft took these images
of dwarf planet Ceres.
The elongated shape
of the dwarf planet is due to its rapid rotational spin, not a lack of mass, which is about one - third that of Pluto.
An artist's depiction
of the dwarf planet Ceres.
The observations taken during the occultation also gave more accurate details
of the dwarf planet's size, showing it to be an oblate spheroid measuring 1,430 km by 1,500 km, making it about two - thirds the size of Pluto.