fr en es pt
astronomy
 
 
 
 
 
 
      RSS astronoo   about   google+    
 

Dwarf planets

Dwarf planets

 Automatic translationAutomatic translation Category: Planets and dwarf planets
Updated June 01, 2013

"A planet is a celestial body which is on orbit around the Sun, which possesses a sufficient mass so that its gravity takes it on the strengths of cohesion of the solid body and maintains it in hydrostatic equilibrium (spherical shape), and which eliminated any body moving on a close orbit ".
This definition was approved on August 24th, 2006, during the 26th General assembly of the UAI (International Astronomical Union) by a vote by a show of hands about 400 scientists and astronomers after ten days of discussions. In addition, the UAI created a new class of objects: the dwarf planets. A dwarf planet, since the new definition of August, 2006, is a celestial body on orbit around the Sun:
- witch has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (near-spherical) shape,
- witch has not cleared the neighborhood around its orbit.
- witch is not a satellite
According to this last one, three bodies reach the status of dwarf planet: Pluto, Eris, and Ceres. Other bodies should soon join this nomenclature.

 size of dwarf planets

Image: Representation of the largest trans-Neptunian objects known from the Earth. The four biggest: Eris, Pluto, Makemake and Haumea were granted the status of dwarf planet.

 
Dwarf planets Orbital period
(km)
Diameter
 (km)
     
Eris 557 2326 ± 12
Pluto 248.90 2306 ± 20
Haumea 283.28 1240 ± 60
Makemake 309.90 1478 ± 17
Sedna ≈ 11400 995 ± 80
Ceres 4.60 974,6 ± 3.2
Orcus 245.18 917 ± 25
Quaoar 285.97 1070 ± 38
Charon 248.90 1207 ± 1.5
2002 TC302 408.03 ≈ 1200
Varuna 283.20 ≈ 936
2002 UX25 277 ≈ 910
2002 TX300 284.69 ≈ 900
Ixion 248.37 ≈ 759
2002 AW197 321 700 ± 50

Pluto

    
Pluto Discovered in 1930 by the American astronomer Clyde Tombaugh, Pluto is out of the ordinary. Of an equatorial diameter lower than 2 500 km, it represents only tenth two of the Earth. Not satisfied to be, so far, the smallest member of the solar system, it also possesses an eccentric and very oblique orbit with regard to the plan of the ecliptic.  was discovered in 1930 during the search for a celestial body allowing to explain the orbitales disturbances of Uranus and Neptune, hypothesis proposed by Percival Lowell as being the Planet X. Pluto possesses a satellite, Charon, discovered by James Christy in 1978, is a big satellite with regard to the planet mother (diameter 1270 km).
Charon has a mass about ten times lower than Pluto and the report of diameters is from 1 to 2.
 PLUTON.jpg (8940 octets)  
Pluto 
  
diameter 2306±20 km
surface 17 millions km²
mass 1,314±0,018×1022 kg
gravity 0,655 m/s²
inclination of the axis119,61°
albedo 0,60
escape velocity1,3 km/s
absolute magnitude  
rotation period 
surface temperature33 K à 55 K

Eris

    
Eris The object 2003UB313, is officially appointed by the international astronomical Union in August, 2006. The name chooses is that of the Greek goddess Eris. In the Greek mythology, Eris is the goddess of the Discord. According to Hésiode, she is a girl of Nyx (the Night) and a mother of the Pain, the Famine and the other plagues  was photographed for the first time during made observations in October 21st, 2003 with the telescope Oschin of 1,22 meters of the Mountain Palomar, in California, by the team of Caltech was photographed for the first time during observations made which had already discovered several big beyond Neptune objects as (50000) Quaoar and (90377) Sedna.
Thanks to the spatial telescope Hubble and to that of the W.M. Keck Observatory the measure of the mass of Eris, the biggest member of the class of dwarfish planets in our Solar system, was able to be realized. Eris is 1,27 times as massive as Pluto, formerly the biggest member of the Belt of Kuiper of the ice-cold objects revolving beyond the orbit of Neptune.
 Eris et dysnomie 
Eris 
  
diameter 2 400 km ± 100 km
surface  
mass 1,668×1022 kg
gravity  
inclination of the axis 
albedo 0,6 
liberation speed 
absolute magnitude -1,2
rotation period 
surface temperature≈ 30 K

Ceres

    
Ceres Ceres is the first bare asteroid. We recognize him the definition of dwarfish planet today, since the new definition of the international astronomical Union of August, 2006. With about a diameter 950 km, Ceres is also the biggest member of the belt of asteroids situated between the orbits of Mars and Jupiter was accidentally discovered.
Piazzi tried to observe a star listed by Francis Wollaston under the name of Mayer 87 because she was not in the position given in the zodiacal catalog of Mayer (it turned out afterward that it was in fact about Lacaille 87).
On the place, he observed an object moving on the sky, that he believed at first to be a comet.

Image: Ceres view from the Hubble Space Telescope (ACS). The contrasts were raised to reveal the details of the surface. Credit NASA, ESA

 dwarf planet Ceres  
Ceres 
  
diameter 959,2×932,6 km
surface  
mass 9,445×1020 kg
gravity 0,26 m/s²
inclination of the axis 
albedo 0,113
liberation speed0,51 km/s
absolute magnitude 3,34
rotation period0,3781 d
surface temperature≈167 K

Haumea

    

Haumea is one of the largest members of a family called TNO (Trans-Neptunian Object).
This object called 2003 EL61 first because his first appearance on a photograph from 2003, was officially named by the International Astronomical Union: Haumea.
Haumea is an object transneptunian (OTN) of oblong shape, the largest dimension is between 1 960 and 2500 km. He was ranked Dwarf planet September 17, 2008. The discovery of Haumea is controversial and contested by two teams.
Haumea has two satellites Hi'iaka and Namaka, rotates on itself under 4 h, has an ellipsoidal shape and a high albedo due to its composition of water ice.

 Dwarf planet Haumea 
Haumea 
  
Diameter1 960 à 2 500 km
Surface temperature32±3 K

Image: image artist Haumea and its satellites Hi'iaka and Namaka.
crédit: A. Feild (Space Telescope Science Institute)

Makemake

    

Makemake, after the name of the creator god of humanity in the mythology of Rapa Nui Easter Island, is a trans-Neptunian object (OTN), of a dimension between 1300 and 1900 km. Makemake discovered in 2005 by Michael E. Brown, Chadwick Trujillo and David Rabinowitz of the Caltech almost simultaneously than Eris, is a dwarf planet. This celestial body is one of the largest known objects in the outer solar system.
Makemake is a dwarf planet reddish, probably covered with frozen methane (CH4). The team, led by José Luis Ortiz (Instituto de Astrofísica de Andalucía, CSIC, Spain), combined observations from multiple telescopes using several different observatories in South America to watch Makemake when passed a distant star in April 2011. Publication November 22, 2012 in the journal Nature: "When Makemake passes the star and obscures its light, the star disappears and reappears in a very abrupt, instead of fading and gradually turn back. This means that the small dwarf planet has no significant atmosphere.".
This member of the Kuiper belt, slightly smaller than Pluto, orbiting the Sun in an orbit slightly more distant. It was registered under number 2005 FY9 soon after its discovery by the team of Mike Brown, before getting its present name July 13, 2008. No image of the surface of Makemake has yet been taken, but its surface is covered with methane, ethane, and possibly nitrogen.

 

Its average temperature is very low (≈ 30 K, ≈ -243.2 ° C). Makemake not seem to have the moon, like other major dwarf planets Eris has one, Haumea has two and Pluto five.

Makemakecharacteristics
  
Dimensions 1 400 à 1 500 km
discovered31 mars 2005
Surface temperature≈35 K
Semi-major axis6.846 x 109 km
Perihelion5.807 x 109 km
Aphelion7.885 x 109 km
Eccentricity0.15
Period of revolution3308 years
Average orbital speed4.389 km/s
Inclination29°
Ascending node79.42°
Argument of perihelion245.85°
 Makemake, as seen by the Hubble telescope

Image: Makemake as seen by the Hubble Space .

Sedna

    
Sedna Sedna (Goddess Inuit of the ice-cold oceans of the north pole), is the biggest beyond Neptune object after Pluto and Eris.   Situated in an almost empty space, Sedna is more red and more brilliant than any object of the solar system.
The scientists have not determined the reason of these unique characteristics yet. He could possess the small moon. In April, 2005 a more precise measure of the celestial body allowed to determine a complete rotation speed about 10 hours.
At the time of its discovery, Sedna was the biggest object discovered in the solar system since the discovery of Pluto. Bigger objects (dwarf planets) were since discovered, as Eris.
 orbit of Sedna 
Sedna 
  
diameter 1180×1800 km
surface  
mass 1.7-6.1×1021 kg
gravity  
inclination of the axis11.934°
albedo 0.2
liberation speed0,62-0,95 km/s
absolute magnitude 1.6
rotation period0.42 d
surface temperature≈33 K

Quaoar

    

Quaoar is an object transneptunian (OTN) within the Kuiper belt and has a size greater than half of that of Pluto.
The Kuiper belt consists of objects made of rock and ice orbiting the Sun and located beyond Neptune.
The discovery in June 2002, made ​​by Michael Brown and Chadwick Trujillo of Caltech (Pasadena, USA), tends to confirm the hypothesis that the Kuiper Belt is home dimension objects comparable to Pluto and beyond.
This strengthens the position of classifying Pluto astronomers, not among the planets but among the objects of the Kuiper belt.
The new object, referred to as Quaoar has a diameter of 1250 km.

 

It follows a circular path about 6.3 billion kilometers from the Sun and 1.8 billion kilometers from Neptune. Pluto follows an elliptical path causing it to the inside of the orbit of Neptune and beyond that of Quaoar. Composed half ice and half rock, Quaoar is black, "dirty ice," said Brown.
It was made black by ultraviolet light which has gradually transformed its organic compounds, and since the beginning of the solar system.
The objects of the Kuiper belt is the remains of the time of the formation of planets.

Image: Quaoar, in the Kuiper belt.

 Quaoar, an asteroid transneptunian

See also

     
      
 
star
 
1997-2013 © Astronoo.com - Astronomy, Astrophysics, Evolution and Earth science.
Reproduction prohibited without permission of the author.
Asteroids
Asteroid 2009 DD45
sending us a sign...
 
Diversity of solar system objects
Tourist travel
in the solar system...
 
Charon Pluto's large moon
Charon will be visited
in 2015...
 
gravity according to Einstein
Image of gravity
from Albert Einstein...
 
météorite
Meteorite,
extra-terrestrial object...
 
The Earth-Crossing Asteroids - NEO
Earth-Crossing Asteroids...