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1 d orbits and sizes between that of Earth and Neptune.
2 er-Earth," whereas the other is more akin to Neptune.
3 representative of the interior of Uranus and Neptune.
4 ocks upstream of Jupiter, Saturn, Uranus and Neptune.
5 he Sun before being captured in orbit around Neptune.
6 and in GCR measured by Voyager 2, then near Neptune.
7 elt analogous region out beyond the orbit of Neptune.
8 similar in morphology to those of Uranus and Neptune.
9 ting of solid bodies orbiting the Sun beyond Neptune.
10 retrograde orbit at 14 planetary radii from Neptune.
11 of 30 to 50 km, were presumably captured by Neptune.
12 rge number of bodies orbiting the Sun beyond Neptune.
13 CH4, water, and ammonia, such as Uranus and Neptune.
14 s may be important as they are at Uranus and Neptune.
15 at of Earth (with radius R Earth symbol) and Neptune (about 4R Earth symbol) are now known to be comm
16 eptune-sized Kepler-4b is similar to that of Neptune and GJ 436b, even though the irradiation level i
17 MIF was observed for Si isotopes on both Neptune and Neptune plus MC-ICPMS instruments in this st
19 objects, KBOs) that lie beyond the orbit of Neptune and which are believed to have formed contempora
20 planetary systems (including systems of 'hot Neptunes' and 'super-Earths') whose angular momentum vec
21 ity waves can result in orbital evolution of Neptune as well as changes in the structure of the Kuipe
22 The Kuiper belt extends from the orbit of Neptune at 30 au to an abrupt outer edge about 50 au fro
23 iper belt-the region of space extending from Neptune (at 30 astronomical units) to well over 100 AU a
31 a vast swarm of small bodies orbiting beyond Neptune, have been a major process affecting this popula
32 re likely captured by a migrating, eccentric Neptune in a dynamically excited planetesimal population
33 f two Sun-like stars by planets smaller than Neptune in the billion-year-old open cluster NGC6811.
36 e-temperature brown dwarfs resembles that of Neptune, indicating the presence of zonal temperature an
37 roximately 10(3)-kilometre-sized bodies) and Neptune is a far more likely explanation for Triton's ca
39 Similar populations and dynamics at both Neptune Lagrangian regions indicate that the Trojans wer
40 as massive as Jupiter, to intermediate-mass Neptune-like objects with large cores and moderate hydro
41 far too small to deplete the atmosphere of a Neptune-like planet in the lifetime of the parent star,
42 n that hot rocky planets might have begun as Neptune-like, but subsequently lost all of their atmosph
43 Here we report that in the ultraviolet the Neptune-mass exoplanet GJ 436b (also known as Gliese 436
46 of the Sun) host star, and is one of the few Neptune-mass planets that is amenable to detailed charac
48 e influence of sample introduction system on Neptune MC-ICPMS lead isotopic ratio measurements was te
51 the hundreds of multi-planet systems of sub-Neptunes, more planet pairs are observed near resonances
54 e of apsidal wave interaction with the trans-Neptune population of debris called the Kuiper belt.
55 the properties of lower-mass exoplanets (sub-Neptune) remain largely unconstrained because of the cha
56 al magnetic fields of the planets Uranus and Neptune represent important observables for constraining
57 uggest that geophysical models of Uranus and Neptune require reassessment because chemical reactivity
58 et GJ 436b-which has been labelled as a 'hot Neptune'-reveals itself by the dimming of light as it cr
59 5 au and were subsequently pushed outward by Neptune's 1:2 mean motion resonance during its final pha
60 ar, for a belt eroded out to the vicinity of Neptune's 2:1 resonance at about 48 astronomical units,
62 GCR is further supported by the response of Neptune's atmosphere to an intermittent 1.5- to 1.9-year
66 :1 resonance at about 48 astronomical units, Neptune's eccentricity can damp to its current value ove
69 ontrolled by precipitation of electrons from Neptune's magnetosphere as previously proposed, Triton c
74 same wavelengths in the spectra of Pluto and Neptune's satellite Triton are due to CH4 on their surfa
75 ethylene may be required to explain the hot Neptune's small CH(4)-to-CO ratio, which is at least 10(
77 piters (with slightly larger orbits) and hot Neptune-size candidates do exhibit signatures of additio
79 ar absorption in the atmospheres of smaller (Neptune-sized) planets during transits have revealed onl
80 lt is subject to resonant perturbations from Neptune, so that the transport of angular momentum by de
82 Small planets between the sizes of Earth and Neptune substantially outnumber Jupiter-sized planets.
83 anets intermediate in size between Earth and Neptune ('super-Earths') are among the most common plane
84 oir of icy bodies at and beyond the orbit of Neptune-the Kuiper belt-has opened a new frontier in ast
85 rocky core, befitting the appellation ''mini-Neptunes.'' The gas giant planets occur preferentially a
86 e in two cold reservoirs beyond the orbit of Neptune: the Kuiper Belt (equilibrium temperatures of ap
87 disk of icy bodies that orbit the Sun beyond Neptune; the largest known members are Pluto and its com
89 eport the detection of 2008 LC18, which is a Neptune Trojan in the trailing (L5) Lagrangian region of
91 We estimate that the leading and trailing Neptune Trojan regions have similarly sized populations
95 ort the discovery of five irregular moons of Neptune, two with prograde and three with retrograde orb
96 f critical importance for devising models of Neptune, Uranus, and white dwarf stars, as well as of ex
97 atmospheres of Jupiter, Saturn, Uranus, and Neptune were modeled as shallow layers of turbulent flui
98 e bodies in the universe, such as Saturn and Neptune, where nonmolecular ice is thought to be the mos
99 ere, we identified a novel Xenopus KLF gene, neptune, which is highly expressed in the ventral blood
100 jects orbiting primarily between Jupiter and Neptune--with an equivalent radius of 124 +/- 9 kilometr
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