Well, this 100 000 year cycle is the ECCENTRICITY CYCLE of the Earth Orbit around the Sun: The orbit oscillates between a more elliptical and
a more circular orbit every (approximately) 100 000 years.
This cycle coincides with a change in Earth's orbit as it evolves from
a more circular orbit to a more elliptical orbit.
The planet is in a binary star system, so it might also be the case that the second star in the binary made a close approach that threw HD 20782 off
a more circular orbit.
Only objects in
more circular orbits have low enough relative velocities to coalesce.
Not exact matches
The Earth's axis wobbles or «precesses» on a 26,000 - year cycle; it changes its average tilt on a 41,000 - year cycle; and it shifts its
orbit from being roughly
circular to
more elliptical on a 100,000 - year cycle.
What's
more, multi-planet systems tend to have
circular orbits all in the same plane, and singletons»
orbits tend to be elliptical and tilted.
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.
Since the tidal effect is strongest when the moon is closest to the primary, it also tends to make the
orbit more circular.
What's
more, the close, roughly
circular orbits of Phobos and Deimos are inconsistent with the idea that they were once asteroids that were strong - armed into joining the Martian family by the Red Planet's gravitational clout.
There is evidence that Earth has gone through at least one globally frozen, «snowball» state in the last billion years, which i... ▽
More Although the Earth's
orbit is never far from
circular, terrestrial planets around other stars might experience substantial changes in eccentricity that could lead to climate changes, including possible «phase transitions» such as the snowball transition (or its opposite).
CFEPS Larger image For an Edgeworth - Kuiper object (EKO), 2004 XR 190 («Buffy») has an unusually
circular orbit (
more).
Planet c may have a minimum mass around 54 + / - 0.7 percent of the mass of Jupiter with a semi-major axis of 3.6 + / -0.1 AUs and a roughly
circular orbit (0.10 +0.5 / -0.1) that takes
more than 6.5 years (2,391 +100 / -87 days) to complete (Gregory and Fischer, 2010; and Fischer et al, 2001 — in pdf).
The planet is comparable to Saturn in mass and size, and is on a nearly
circular 229 - day
orbit around its two p... ▽
More We report the detection of a planet whose
orbit surrounds a pair of low - mass stars.
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.
The four distinguishing characteristics of the spirals are: (a) they have
more orderly, rotational motion than random motion (the rotation refers to the disk as a whole and means that the star
orbits are closely confined to a narrow range of angles and are fairly
circular); (b) they have some or a lot of gas and dust between the stars; (c) this means they can have new star formation occuring in the disk, particularly in the spiral arms; and (d) they have a spiral structure.
Given what an important breakthrough it was for Kepler to realize, and convince others, that the movements of the planets were not constrained to divinely perfect circles, it's kind of surprising that now we have a case where uniform
circular orbits are apparently the
more physically valid solution and elliptical
orbits are the solution being forced by selectively discarding data.
That means that the belt's biggest bodies... would never have formed unless they originally followed
more circular, low - inclination
orbits.
Wikipedia (that «highly reliable font of wisdom») says «The Copernican system was no
more accurate than Ptolemy's system, because it still used
circular orbits.
Those arguing that Earth should be
orbiting about the solar system's barycenter seem to be assuming that a (
more or less)
circular orbit about the barycenter should be possible.
MILANKOVITCH CYCLES overall favor N.H. cooling and an increase in snow cover over N.H high latitudes during the N.H summers due to the fact that perihelion occurs during the N.H. winter (highly favorable for increase summer snow cover), obliquity is 23.44 degrees which is at least neutral for an increase summer N.H. snow cover, while eccentricity of the earth's
orbit is currently at 0.0167 which is still
circular enough to favor reduced summertime solar insolation in the N.H. and thus promote
more snow cover.
Our
orbit is also
more circular at some times (repeating at about 100,000 and 400,000 years), making the month - of - closest - approach factor periodically less important.