1,503 research outputs found
Pencil-Beam Surveys for Faint Trans-Neptunian Objects
We have conducted pencil-beam searches for outer solar system objects to a
limiting magnitude of R ~ 26. Five new trans-neptunian objects were detected in
these searches. Our combined data set provides an estimate of ~90
trans-neptunian objects per square degree brighter than ~ 25.9. This estimate
is a factor of 3 above the expected number of objects based on an extrapolation
of previous surveys with brighter limits, and appears consistent with the
hypothesis of a single power-law luminosity function for the entire
trans-neptunian region. Maximum likelihood fits to all self-consistent
published surveys with published efficiency functions predicts a cumulative sky
density Sigma(<R) obeying log10(Sigma) = 0.76(R-23.4) objects per square degree
brighter than a given magnitude R.Comment: Accepted by AJ, 18 pages, including 6 figure
Constraints on the Orbital Evolution of Triton
We present simulations of Triton's post-capture orbit that confirm the
importance of Kozai-type oscillations in its orbital elements. In the context
of the tidal orbital evolution model, these variations require average
pericenter distances much higher than previously published, and the timescale
for the tidal orbital evolution of Triton becomes longer than the age of the
Solar System. Recently-discovered irregular satellites present a new constraint
on Triton's orbital history. Our numerical integrations of test particles
indicate a timescale for Triton's orbital evolution to be less than yrs
for a reasonable number of distant satellites to survive Triton's passage. This
timescale is inconsistent with the exclusively tidal evolution (time scale of
yrs), but consistent with the interestion with the debris from
satellite-satellite collisions. Any major regular satellites will quickly
collide among themselves after being perturbed by Triton, and the resulting
debris disk would eventually be swept up by Triton; given that the total mass
of the Uranian satellite system is 40% of that of Triton, large scale evolution
is possible. This scenario could have followed either collisional or the
recently-discussed three-body-interaction-based capture.Comment: 10 pages, 4 figures, accepted for ApJ
A Possible Divot in the Size Distribution of the Kuiper Belt's Scattering Objects
Via joint analysis of a calibrated telescopic survey, which found scattering
Kuiper Belt objects, and models of their expected orbital distribution, we
measure the form of the scattering object's size distribution. Ruling out a
single power-law at greater than 99% confidence, we constrain the form of the
size distribution and find that, surprisingly, our analysis favours a very
sudden decrease (a divot) in the number distribution as diameters decrease
below 100 km, with the number of smaller objects then rising again as expected
via collisional equilibrium. Extrapolating at this collisional equilibrium
slope produced enough kilometer-scale scattering objects to supply the nearby
Jupiter-Family comets. Our interpretation is that this divot feature is a
preserved relic of the size distribution made by planetesimal formation, now
"frozen in" to portions of the Kuiper Belt sharing a "hot" orbital inclination
distribution, explaining several puzzles in Kuiper Belt science. Additionally,
we show that to match today's scattering-object inclination distribution, the
supply source that was scattered outward must have already been vertically
heated to of order 10 degrees.Comment: accepted 2013 January 8; published 2013 January 22 21 pages, 4
figure
Consequences of a Distant Massive Planet on the Large Semi-major Axis Trans-Neptunian Objects
We explore the distant giant planet hypothesis by integrating the large
semi-major axis, large pericenter Trans-Neptunian Objects (TNOs) in the
presence of the giant planets and an external perturber whose orbit is
consistent with the proposed distant, eccentric, and inclined giant planet, so
called planet 9. We find that TNOs with semi-major axes greater than 250 au
experience some longitude of perihelion shepherding, but that a generic outcome
of such evolutions is that the TNOs evolve to larger pericenter orbits, and
commonly get raised to retrograde inclinations. This pericenter and inclination
evolution requires a massive disk of TNOs (tens of M_\Earth) in order to
explain the detection of the known sample today. Some of the highly inclined
orbits produced by the examined perturbers will be inside of the orbital
parameter space probed by prior surveys, implying a missing signature of the
9th planet scenario. The distant giant planet scenarios explored in this work
do not reproduce the observed signal of simultaneous clustering in argument of
pericenter, longitude of the ascending node, and longitude of perihelion in the
region of the known TNOs
Using long-term transit timing to detect terrestrial planets
We propose that the presence of additional planets in extrasolar planetary
systems can be detected by long-term transit timing studies. If a transiting
planet is on an eccentric orbit then the presence of another planet causes a
secular advance of the transiting planet's pericenter over and above the effect
of general relativity. Although this secular effect is impractical to detect
over a small number of orbits, it causes long-term differences in when future
transits occur, much like the long-term decay observed in pulsars. Measuring
this transit-timing delay would thus allow the detection of either one or more
additional planets in the system or the first measurements of non-zero
oblateness () of the central stars.Comment: 10 pages, 5 figures, accepted by Monthly Notices, updated to reflect
accepted versio
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