However, the development of an Earth - like planet in this zone could have been disrupted by
the eccentric orbit of planet b. Astronomers would find it very difficult to detect an Earth - type planet in the water zone of this star using present methods.
Not exact matches
Another surprise is that a number
of these big
planets are on fairly
eccentric orbits, not circular like those
of Jupiter and Earth.
An earlier observation
of HD 20782 suggested that the
planet might have an extremely
eccentric orbit.
It has an
eccentric orbit that is highly inclined with respect to the
planets and takes it closer to the Sun than Neptune during a portion
of its
orbit.
It
orbits around the star 70 Virginis in a highly
eccentric, or oval, path quite unlike those
of the familiar
planets.
The only known transiting
planet with a comparably long
orbit, called HD 80606 b, has an extremely
eccentric orbit; the distance between HD 80606 b and its star varies greatly throughout the
planet's
orbit, driving temperature changes
of several hundred degrees in a matter
of hours.
None resemble the former ninth
planet, which also has a distinctly
eccentric, or elliptical,
orbit that crosses that
of Neptune.
However, the inner,
eccentric orbit of a giant planetary companion «b» recently discovered around 54 Piscium would probably disturb the
orbit of such an Earth - type
planet.
The Fomalhaut team led by Paul Kalas (University
of California, Berkeley) considers this circumstantial evidence that there may be other
planet - like bodies in the system that gravitationally disrupted Fomalhaut b to place it in such a highly
eccentric orbit.
At the January 2002, 199th Meeting
of the American Astronomical Society in Washington, DC, two teams
of astronomers announced that the cold dust in Vega's circumstellar disk is at least partly gathered into large clumps, in a characteristic shape that suggests the gravitational influence
of a giant
planet in an
eccentric orbit (Abstracts for sessions 66.04 and 66.05, and CfA press release).
We show that a giant
planet on a sufficiently
eccentric orbit can excite extreme eccentricity oscillations in the
orbit of a habitable terrestrial
planet.
In particular, I will focus on
planets on
eccentric orbits, not only because typical exoplanetary systems have been found to contain these, but also because their interactions with debris disks theoretically facilitates the transport
of icy bodies within the habitable zone
of planetary systems.
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.
We find that this standard ansatz provides a reasonable lower bound on the outer boundary
of the habitable zone, but the influence
of obliquity and ocean fraction can be profound in the context
of planets on
eccentric orbits.
The same data can argue for different numbers
of planets depending on whether you assume
eccentric (highly elliptical)
orbits or nearly circular ones.
That cluster is also devoid
of the heavy chemical elements thought necessary to evolve a
planet.8 At least 30 separate
planets each
orbit a pair
of suns whose constantly changing positions would disrupt any slow evolution
of a
planet.9 One
planet has been repeatedly observed eclipsing each
of the
eccentric binary stars it
orbits.
The
orbit of object «b» around 79 Ceti is only mildly
eccentric, but may still be more elliptical than that
of any
planet in the Solar System other than Pluto.
A comparison
of stellar densities from asteroseismology with densities derived from transit models in Batalha et al. assuming circular
orbits shows significant disagreement for more than half
of the sample due to systematics in the modeled impact parameters, or due to
planet candidates which may be in
eccentric orbits.
On March 26, 2014, astronomers announced the discovery
of another dwarf
planet in a highly
eccentric orbit like Sedna.
Now, remember that we postulated a very
eccentric orbit, this means that the tidal effect will vary greatly and be much larger when the
planet is closest to the star, hence if tides can interfere with or perhaps even control generation
of star spots, then the generation
of the activity would be synchronized with the orbital period
of the star.
It therefore seems likely that exotic cases
of highly
eccentric orbits may be prominent in other solar systems, where various gaseous
planets are known to exhibit large orbital fluctuations.