The orbital planes of planets «c» and «d» around Star A are inclined at 30 degrees to each other (more).
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.
Oddly enough, Oort Cloud objects were probably formed in a region of the proto - planetary disk that was located closer to the Sun than the Edgeworth - Kuiper Belt objects that persist in
the orbital plane of the planets (ecliptic) to this day.
Not exact matches
Axial tilt is an astronomical term regarding the inclination angle
of a
planet's rotational axis in relation to a perpendicular to its
orbital plane.
The axial tilt may equivalently be expressed in terms
of the
planet's
orbital plane and a
plane perpendicular to its axis.
The team's calculations also suggest two likely
orbital planes for the
planet: one moderately close to the mean
plane of the solar system and near the mean
plane of the four eKBOs at about 18 degrees, and one steeper
plane, inclined at about 48 degrees.
The tilt
of the solar system's
orbital plane has long befuddled astronomers because
of the way the
planets formed: as a spinning cloud slowly collapsing first into a disk and then into objects orbiting a central star.
«The
planets are small, they have circular orbits, their
orbital planes are flat — it starts to look like home very quickly,» says Jason Rowe
of the SETI Institute in Mountain View, California.
In 2006, astronomers discovered a very dim («mid-range»), red dwarf companion to HD 189733 A
of spectral and luminosity type M V. Observed at a separation
of 216 AUs from Star A, the companion star has a clockwise orbit that is nearly perpendicular to the
orbital plane of transiting
planet b around Star A (HD 189733 b or Ab).
The different Q values also allow the
planets to re-align their orbits with the spin
of the star (so that the
orbital plane is perpendicular to the star's spin axis) on a timescale shorter than the
orbital period decay, thus explaining why there are many «aligned» hot Jupiters.
«We expect each
of the KBOs»
orbital tilt angle to be at a different orientation, but on average, they will be pointing perpendicular to the
plane determined by the sun and the big
planets,» she added.
That
Planet Nine helps to explain the tilt of the solar system's orbital plane is another vote of confidence for the planet's exis
Planet Nine helps to explain the tilt
of the solar system's
orbital plane is another vote
of confidence for the
planet's exis
planet's existence.
Obliquity is the angle
of a
planet's axis
of rotation relative to its
orbital plane.