47 Ursae Majoris b
2007 Schools Wikipedia Selection. Related subjects: Space (Astronomy)
| Extrasolar planet | Lists of extrasolar planets | |
|---|---|---|
| Parent star | ||
| Star | 47 Ursae Majoris | |
| Constellation | Ursa Major | |
| Right ascension | (α) | 10h 59m 28.0s |
| Declination | (δ) | +40° 25′ 49″ |
| Spectral type | G1V | |
| Orbital elements | ||
| Semimajor axis | (a) | 2.13 ± 0.12 AU |
| Eccentricity | (e) | 0.061 ± 0.014 |
| Orbital period | (P) | 1089.0 ± 2.9 d |
| Inclination | (i) | ?° |
| Longitude of periastron |
(ω) | 172 ± 15° |
| Time of periastron | (τ) | 2,450,356 ± 34 JD |
| Physical characteristics | ||
| Mass | (m) | >2.63 ± 0.23 MJ |
| Radius | (r) | ? RJ |
| Density | (ρ) | ? kg/ m3 |
| Temperature | (T) | ? K |
| Discovery information | ||
| Discovery date | 1996 | |
| Discoverer(s) | Marcy, Butler et al. | |
| Detection method | Doppler Spectroscopy | |
| Discovery status | Confirmed | |
47 Ursae Majoris b is an extrasolar planet orbiting the Sun-like star 47 Ursae Majoris. It is located in a long- period, near-circular orbit and is the innermost known planet in its planetary system. 47 Ursae Majoris b was discovered in 1996 and has a mass at least 2.63 times that of Jupiter.
Discovery
Like the majority of known extrasolar planets, 47 Ursae Majoris b was discovered by detecting the changes in its star's radial velocity as the planet's gravity pulls the star around. This was achieved by observing the Doppler shift of the spectrum of 47 Ursae Majoris. After the discovery of the first extrasolar planet around a Sun-like star, 51 Pegasi b, astronomers Geoffrey Marcy and R. Paul Butler searched through their observational data for signs of extrasolar planets and soon discovered two: 47 Ursae Majoris b and 70 Virginis b. The discovery of 47 Ursae Majoris b was announced in 1996.
Orbit and mass
47 Ursae Majoris b orbits at a distance of 2.13 AU from its star, taking 1,089 days to complete a revolution. It was the first long-period planet around a main sequence star to be discovered. Unlike the majority of known long-period extrasolar planets, the eccentricity of the orbit of 47 Ursae Majoris b is low. The planet lies close to a 2:5 orbital resonance with the outer planet 47 Ursae Majoris c, a similar configuration to Jupiter and Saturn in our solar system. In addition, the ratio of the masses of the two planets is similar to the mass ratio of Jupiter and Saturn.
A limitation of the radial velocity method used to detect 47 Ursae Majoris b is that only a lower limit on the planet's mass can be obtained. Preliminary astrometric measurements suggest the planet's orbit is inclined at an angle of 63.1° to the plane of the sky. If confirmed, this would imply the true mass of the planet is around 2.9 times that of Jupiter. In any case, the mass cannot be much greater than the lower limit or the system would be unstable.
Characteristics
Given the planet's high mass, it is likely that 47 Ursae Majoris b is a gas giant with no solid surface. Since the planet has only been detected indirectly, properties such as its radius, composition and temperature are unknown. Assuming a composition similar to that of Jupiter and an environment close to chemical equilibrium, the upper atmosphere of the planet is expected to contain water clouds, as opposed to the ammonia clouds typical of Jupiter.
While 47 Ursae Majoris b lies outside its star's habitable zone, its gravitational influence would disrupt the orbit of planets in the outer part of the habitable zone. In addition, it may have disrupted the formation of terrestrial planets and reduced the delivery of water to any inner planets in the system. Therefore planets located in the habitable zone of 47 Ursae Majoris are likely to be small and dry.
47 Ursae Majoris b in fiction
The Coyote series by Allen Steele is mainly set on Coyote, a fictional habitable moon of 47 Ursae Majoris b, which is named Bear in the books.