» Extrasolar Planet Guide » upsilon Andromedae » upsilon Andromedae d


Water Cloud Jovian, Eccentric

Object Type: Water Cloud Jovian, Eccentric
Parent Star: upsilon Andromedae (F8 V)
Discovery Status: Confirmed
Habitability: Planet at outer edge of Habitable Zone at Mean Orbital Distance
Orbit of upsilon Andromedae d Current Planet
Habitability Zone Habitability Zone
Mass ( M sin i ): 3.75 Jupiters
Periastron Distance: 1.84 AU
Mean Distance: 2.53 AU
Apastron Distance: 3.21 AU
Orbital Period: 1284 ± 30 Days
Eccentricity: 0.27 ± 0.11
Argument of Perihelion (omega):
260 °
Radial Velocity of Star: 69.5 m/s
System Age: 5000 Myr
Planet Appearance:
White water ice clouds
Estimated Radius:
1.039 Jupiters 1
Estimated Periastron Temp: 254 Kelvin
Estimated Mean Temp: 217 Kelvin
Estimated Apastron Temp: 192 Kelvin
Temp from
Internal Heating :

171.492 Kelvins 2
Max Angular Star Size: 0.479°
Mean Angular Star Size: 0.349°
Min Angular Star Size: 0.275°
Gravitational Influence
(Hill Sphere):
0.243 AU / 36410000 km
Max Stable Prograde Moon Orbit: 0.087 AU / 13100000 km
Max Moon Mass: > 10 Earths 3
Tidally locked if older than: > 20 Gyr 4
Estimated Bond Albedo: ~ 0.84 5
Notes:
     1 from planet formation models of Burrows et al
     2 from planet formation models of Burrows et al
     3 based on periastron due to high eccentricity
     4 orbit may be too eccentric for 1:1 tidal lock
     5 from Sudarsky et al. 2000
Year Discovered: 1999
Detection Method: Doppler Spectroscopy
Discovered By: Marcy and Butler



Upsilon Andromedae made history recently with the discovery that the star parented not just one planet, but three. It was the first multiplanet solar system to be discovered around a sun-like star.

Weighing in at 4 Jupiter masses is upsilon Andromedae d, the outermost known planet in this new solar system. At an average distance of 2.5 AUs, this world is has a larger orbit than Mars. The planet would likely have total cloud cover and look quite similar to Jupiter. It’s moons could be quite massive and would be mostly rocky worlds with large amounts of ice. Some of these moons may have vast tracks of their icy surfaces melted and featureless. Recent studies indicate that stars with epistellar planets, like upsilon Andromedae b, might emit superflares every century or so. If this is happening within the upsilon Andromedae system, then great areas of the icy moons of the outermost planet may have been melted smooth by these titanic stellar eruptions.

Imagine floating above the main cloud deck of water ice clouds at the equator of upsilon Andromedae d. On the horizon, the sun is setting. Bisecting our view, we see the rings of the third planet as a thin line, glowing in the waning light. The shadow of the rings paints a dark swath on the cloud tops below. Within the rings, small shepherd moons glow like tiny diamonds. The planet’s larger more distant moons can be seen arrayed in line with the rings. In the distance, two bright stars defy the light of the setting sun. These are the first and second planets of upsilon Andromedae.


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Sunset on Upsilon Andromedae d
On the equator of gas giant upsilon Andromedae d, we float above the main cloud deck of water ice clouds. On the horizon, the sun is setting. Bisecting our view, we see the rings of the third planet as a thin line, glowing in the waning light. The shadow of the rings paints a dark swath on the cloud tops below. Within the rings, small shepherd moons glow like tiny diamonds. The planet’s larger more distant moons can be seen arrayed in line with the rings. In the distance, two bright stars defy the light of the setting sun. These are the first and second planets of upsilon Andromedae.


View the Night Sky from upsilon Andromedae d...

Cylindrical All Sky View
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Northern Hemisphere
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Southern Hemisphere
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