Dwarf Planets - Official and Nearly Certain Dwarf Planets

Official and Nearly Certain Dwarf Planets

As of 2011, five objects are recognized as dwarf planets by the IAU. Mike Brown considers these and four others to be "nearly certain". For Ceres and Pluto, this is known through direct observation. Brown thinks the other seven are massive enough to be in hydrostatic equilibrium even if they are dense (primarily rocky) and at the lower end of their estimated diameters. Eris is more massive than Pluto; Haumea and Makemake were assigned names as dwarf planets based on their absolute magnitudes. In relative distance from the Sun, the five "official" dwarf planets are:

  1. Ceres – discovered on January 1, 1801, 45 years before Neptune. Considered a planet for half a century before reclassification as an asteroid. Accepted as a dwarf planet by the IAU on September 13, 2006.
  2. Pluto – discovered on February 18, 1930. Classified as a planet for 76 years. Reclassified as a dwarf planet by the IAU on August 24, 2006.
  3. Haumea – discovered on December 28, 2004. Accepted by the IAU as a dwarf planet on September 17, 2008.
  4. Makemake – discovered on March 31, 2005. Accepted by the IAU as a dwarf planet on July 11, 2008.
  5. Eris – discovered on January 5, 2005. Called the "tenth planet" in media reports. Accepted by the IAU as a dwarf planet on September 13, 2006.

The other four "nearly certain" objects per Brown, Tancredi, et al. are:

  1. Orcus – discovered on February 17, 2004.
  2. Quaoar – discovered on June 5, 2002.
  3. 2007 OR10 – discovered on July 17, 2007.
  4. Sedna – discovered on November 14, 2003.

No space probes have visited any of these. This will change if NASA's Dawn and New Horizons missions reach Ceres and Pluto, respectively. The plans are for Dawn to orbit Ceres, and New Horizons to fly by Pluto, both in 2015. Dawn entered orbit around the potential dwarf planet Vesta on 16 July 2011. On 5 September 2012, Dawn left Vesta in order to orbit Ceres, which it is scheduled to reach in February 2015.

Objects recognized by the IAU as dwarf planets
Orbital attributes
Name Region of
Solar System
Orbital
radius (AU)
Orbital period
(years)
Mean orbital
speed (km/s)
Inclination
to ecliptic
Orbital
eccentricity
Planetary
discriminant
Ceres Asteroid belt 2.77 4.60 17.882 10.59° 0.079 0.33
Pluto Kuiper belt (plutino) 39.48 248.09 4.666 17.14° 0.249 0.077
Haumea Kuiper belt (12:7) 43.13 283.28 28.22° 0.195 0.020
Makemake Kuiper belt (cubewano) 45.79 309.9 4.419 28.96° 0.159 0.02
Eris Scattered disc 67.67 557 3.436 44.19° 0.442 0.10
Physical attributes
Name Equatorial
diameter
relative to
the Moon
Equatorial
diameter
(km)
Mass
relative to
the Moon
Mass
(×1021 kg)
Density
(g/cm3)
Surface
gravity
(m/s2)
Escape
velocity
(km/s)
Axial
inclination
Rotation
period
(days)
Moons Surface
temp.
(K)
Atmosphere
Ceres 28% 974.6±3.2 1.3% 0.94 2.08 0.27 0.51 ≈ 3° 0.38 0 167 none
Pluto 66% 2306±20 17.8% 13.05 2.0 0.58 1.2 119.59° −6.39 5 44 transient
Haumea ≈ 37% 1300±? 5.5% 4.01 ± 0.04 2.6–3.3 (?) 0.44 0.84 0.16 2 32 ± 3 ?
Makemake 41% 1420±60 ≈ 4% ? ≈ 3 ? 1.7 ± 0.3 ? 0.32 0 ≈ 30 none
Eris 67% 2326±12 22.7% 16.7 2.5 ≈ 0.8 1.3 ≈ 1 (0.75–1.4) 1 ≈ 42 transient?
Objects recognized by others as dwarf planets
Orbital attributes
Name Region of
Solar System
Orbital
radius (AU)
Orbital period
(years)
Mean orbital
speed (km/s)
Inclination
to ecliptic
Orbital
eccentricity
Planetary
discriminant
Orcus Kuiper belt (plutino) 39.17 245.18 20.57° 0.227 0.003
Quaoar Kuiper belt (cubewano) 43.405 285.97 8.00° 0.039 0.007–0.010
2007 OR10 Scattered disc (10:3?) 67.21 550.98 30.70° 0.500 ?
Sedna Detached 518.57 ≈11,400 11.93° 0.853 ?
Physical attributes
Name Equatorial
diameter
relative to
the Moon
Equatorial
diameter
(km)
Mass
relative to
the Moon
Mass
(×1021 kg)
Density
(g/cm3)
Surface
gravity
(m/s2)
Escape
velocity
(km/s)
Axial
inclination
Rotation
period
(days)
Moons Surface
temp.
(K)
Atmosphere
Orcus ≈ 22% 760–810 0.9% 0.63 ° 0.55 1
Quaoar ≈ 26% 890±70 1.8–2.6% 1.6 ± 0.3 ° 0.74 1
2007 OR10 ≈ 37% 1280±210 ? ? ? 0
Sedna ≈ 30% 995 ± 80 ≈1.4% ≈1 ? 0.42 0 ≈ 12

Read more about this topic:  Dwarf Planets

Famous quotes containing the words official, dwarf and/or planets:

    We were that generation called “silent,” but we were silent neither, as some thought, because we shared the period’s official optimism nor, as others thought, because we feared its official repression. We were silent because the exhilaration of social action seemed to many of us just one more way of escaping the personal, of masking for a while that dread of the meaningless which was man’s fate.
    Joan Didion (b. 1935)

    A dwarf who brings a standard along with him to measure his own size—take my word, is a dwarf in more articles than one.
    Laurence Sterne (1713–1768)

    Marriage is the clue to human life, but there is no marriage apart from the wheeling sun and the nodding earth, from the straying of the planets and the magnificence of the fixed stars.
    —D.H. (David Herbert)