- An
apsis (from
Ancient Gr**** ἁψίς (hapsís) 'arch, vault'; pl. apsides /ˈæpsɪˌdiːz/ AP-sih-deez) is the ****hest or
nearest point in the
orbit of a planetary...
- The
scattered ETNOs (or
extreme scattered disc objects, ESDOs) have
perihelia around 38–45 AU and an
exceptionally high
eccentricity of more than 0...
- Mercury's (0.4667 AU) and
perihelia inside Mercury's (0.3075 AU),
whereas those listed here as
outer grazers have
perihelia within Mercury's aphelion...
- the
giant planets,
predominantly Neptune.
Detached objects have
larger perihelia than
these other TNO po****tions,
including the
objects in
orbital resonance...
-
inclined (inclination 40°) orbit. Like
Planet Nine it
would cause the
perihelia of
objects with semi-major axes
greater than 300 AU to oscillate, delivering...
-
objects of the same size
because they come
nearer to Earth, some
having perihelia around 20 AU.
Several are
known with g-band
absolute magnitude below 9...
- long
timescales exchanges of
angular momentum with
Planet Nine
cause the
perihelia of anti-aligned
objects to rise
until their precession reverses direction...
-
eccentricities ranging as high as 0.8,
inclinations as high as 40°, and
perihelia greater than 30
astronomical units (4.5×109 km; 2.8×109 mi).
These extreme...
- of Neptune's
early outward migration. Most
scattered disc
objects have
perihelia within the
Kuiper belt but
aphelia far
beyond it (some more than 150 AU...
- rock/electronic
group Detached objects,
objects which have
orbits whose perihelia are
sufficiently distant from the
influence of
Neptune so that they are...
