While multiple -
planet systems tend to have circular orbits that all lie in the same plane — like our solar system — the orbits of singletons tend to be more elliptical and are often misaligned with the spins of their stars.
Not exact matches
Over time, the rings spread out, and the icy bits that drifted farthest from Saturn eventually reached distances where their gravitational attraction for each other could overcome the
planet's tidal forces that
tended to rip them apart — a process that is still happening today, according to observations by the Cassini spacecraft now touring the Saturn
system.
Astronomers have discovered that stars containing low amounts of the element lithium
tend to host solar
systems, a result that could dramatically reduce the time it will take to detect another Earth - like
planet.
Detecting a habitable
planet is an enormous challenge due to the brightness of the planetary
system's host star, which
tends to overwhelm the relatively dim
planets.
Planets in our solar
system tend to have circular orbits and lie in the same plane.
Its ability to detect
planets on the other side of the galaxy has revamped our understanding of how solar
systems form, which types of stars
tend to pair with which types of
planets, and shed light on the early dynamics of solar
system formation.
In contrast, true transiting
planets would appear clustered around a smaller number of Kepler targets if detectable
planets tend to come in
systems and / or if the orbital planes of
planets encircling the same star are correlated.
This result, that
systems with multiple transiting
planets are less likely to include a transiting giant
planet, suggests that close - in giant
planets tend to disrupt the orbital inclinations of small
planets in flat
systems, or maybe even to prevent the formation of such
systems in the first place.