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1 proximately 40 per cent greater than that of Pluto).
2 tains a warm ice conductive ice shell unlike Pluto.
3 cesses, of a type and scale so far unique to Pluto.
4 ions are accelerated and/or deflected around Pluto.
5  as a result of volatile transport cycles on Pluto.
6 uction of an extensive haze that encompasses Pluto.
7 stimated present-day heat-flow conditions on Pluto.
8 ely replicate the observed fault networks on Pluto.
9 sulting reorientation (true polar wander) of Pluto.
10 x 10(22) kilograms, or 1.27 +/- 0.02 that of Pluto.
11 s a result of a giant impact with primordial Pluto.
12 k Planitia is a nitrogen-ice-filled basin on Pluto(1).
13 s spacecraft in the Tartarus Dorsa region of Pluto (220 degrees -250 degrees E, 0 degrees -20 degrees
14                                              Pluto also has ancient cratered terrains up to ~4 billio
15                 Impact crater populations on Pluto and Charon are not consistent with the steepest im
16   Here we show that P1 and P2's proximity to Pluto and Charon, the fact that P1 and P2 are on near-ci
17  have masses that are small compared to both Pluto and Charon-that is, between 5 x 10(-4) and 1 x 10(
18  spectra across the encounter hemispheres of Pluto and Charon.
19 acecraft has revealed the complex geology of Pluto and Charon.
20  orthogonal to the common pole directions of Pluto and Charon.
21 ould have shaped other methane reservoirs on Pluto and help explain the appearance of the bladed terr
22                        Triton is as large as Pluto and is postulated to have been captured from helio
23 eyond Neptune; the largest known members are Pluto and its companion Charon.
24 round the central 'binary planet' comprising Pluto and its large moon, Charon.
25                                              Pluto and its moon, Charon, are the most prominent membe
26              The physical characteristics of Pluto and its moon, Charon, provide insight into the evo
27 ore distant satellites of Pluto, reveal that Pluto and its moons comprise an unusual, highly compact,
28  near the same wavelengths in the spectra of Pluto and Neptune's satellite Triton are due to CH4 on t
29 ain N-bearing molecule in the atmospheres of Pluto and Triton and probably the main nitrogen reservoi
30 face appearance and in climate properties on Pluto and Triton, and give further support to the hypoth
31  long-term volatile transport simulations of Pluto and Triton, using the same initial conditions and
32 bserved volatile ice surface distribution on Pluto and Triton.
33                                   Triton and Pluto are believed to share a common origin, both formin
34 nts that measured the space environment near Pluto as it flew by on 14 July 2015.
35 rary cold-trapping of material escaping from Pluto, as well as the photolytic processing of this mate
36 other solar nebula bodies such as Triton and Pluto, but is very different from that of the regular sa
37 e aftermath of a collision that produced the Pluto-Charon binary.
38 otically, driven by the large torques of the Pluto-Charon binary.
39 re used to demonstrate that the formation of Pluto-Charon by means of a large collision is quite plau
40  collisional ejecta that originated from the Pluto-Charon formation event.
41 aracteristics, including ones similar to the Pluto-Charon pair.
42 sitions, and the New Horizons mission to the Pluto-Charon system allows us to test hypotheses on the
43 onsistent with collisional formation for the Pluto-Charon system in which the precursor objects may h
44 der could have moved the feature towards the Pluto-Charon tidal axis, on the far side of Pluto from C
45          This large feature is very near the Pluto-Charon tidal axis.
46 od (about 570 days), very different from the Pluto/Charon system, which was hitherto the only previou
47 years of Charon's formation, ice deposits on Pluto concentrate into a single cap centred near a latit
48                        Observations from the Pluto Energetic Particle Spectrometer Science Investigat
49                                              PLUTO (for plastidic nucleobase transporter) was identif
50  Pluto-Charon tidal axis, on the far side of Pluto from Charon.
51  is possible that a disk of material orbited Pluto from which Charon later accumulated.
52 tions of a proton uncoupler, indicating that PLUTO functions as a proton-substrate symporter.
53  the satellite Charon from its parent planet Pluto, giving separate spectra of the two objects from 1
54                                            A PLUTO green fluorescent protein fusion was shown to resi
55                           Two small moons of Pluto have been discovered in low-eccentricity orbits ex
56 revious searches for other satellites around Pluto have been unsuccessful, but they were not sensitiv
57                   Heterologous expression of PLUTO in an Escherichia coli mutant lacking the bacteria
58 d wavelengths of an occultation of a star by Pluto in August 2002.
59 on a recent model representing conditions on Pluto, in which deepening penitentes reproduce both the
60           The deep nitrogen-covered basin on Pluto, informally named Sputnik Planitia, is located ver
61                                              Pluto is an astoundingly diverse, geologically dynamic w
62                                              Pluto is covered by numerous deposits of methane, either
63 rfacing and a relatively flat surface, while Pluto is not tidally activated and displays a pronounced
64                              We predict that Pluto is therefore several orders of magnitude brighter
65 g that shows that ice quickly accumulates on Pluto near latitudes of 30 degrees north and south, even
66 N2 are inconsistent with the observations on Pluto of non-brittle deformation within the N2-ice sheet
67       The two newly discovered satellites of Pluto (P1 and P2) have masses that are small compared to
68 pparent depletion in volatiles compared with Pluto, perhaps as the result of a more energetic impact.
69  indeed form as a result of an impact and if Pluto possesses a subsurface ocean, the required positiv
70 the discovery of two additional moons around Pluto, provisionally designated S/2005 P 1 (hereafter P1
71  confined sunward of Pluto to within about 6 Pluto radii.
72 on the absence of more distant satellites of Pluto, reveal that Pluto and its moons comprise an unusu
73 These data reveal evidence for extinction in Pluto's atmosphere and show that it has indeed changed,
74                Occultation data acquired for Pluto's atmosphere in 1988 revealed a nearly isothermal
75                                              Pluto's atmosphere is cold and hazy.
76                                              Pluto's atmosphere is highly extended, with trace hydroc
77   It is unclear whether the current state of Pluto's atmosphere is representative of its average stat
78                             We conclude that Pluto's atmosphere is unique among Solar System planetar
79           Another question is to what extent Pluto's atmosphere might be collapsing as it recedes fro
80                                The escape of Pluto's atmosphere provides a potential feedstock for a
81  enhanced-Jeans, hydrodynamic-like escape of Pluto's atmosphere to space.
82  a detailed snapshot of the current state of Pluto's atmosphere.
83 use high-resolution numerical simulations of Pluto's climate to show that the processes forming them
84  averaged over its orbital period, those are Pluto's coldest regions.
85 tly dissipative, which distinguishes it from Pluto's conductive shell.
86                                              Pluto's diverse surface geology and long-term activity r
87                                              Pluto's encounter hemisphere shows ongoing surface geolo
88 iolytically processed volatiles sourced from Pluto's escaping atmosphere.
89                                              Pluto's first known satellite, Charon, was discovered in
90   Here we report observational evidence that Pluto's haze particles are bimodally distributed, which
91 lization of water-ice-rich materials late in Pluto's history.
92  of Sputnik Planitia can substantially alter Pluto's inertia tensor, resulting in a reorientation of
93 existence of these massive features suggests Pluto's interior structure and evolution allows for eith
94 ensation, changing insolation conditions and Pluto's interior structure.
95                                              Pluto's large moon Charon displays tectonics and evidenc
96                          A unique feature of Pluto's large satellite Charon is its dark red northern
97 on near-circular orbits in the same plane as Pluto's large satellite Charon, along with their apparen
98 vered in low-eccentricity orbits exterior to Pluto's large satellite, Charon.
99                                      Charon, Pluto's largest moon, has been extensively studied, with
100 hat is, between 5 x 10(-4) and 1 x 10(-5) of Pluto's mass, and between 5 x 10(-3) and 1 x 10(-4) of C
101 ission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra.
102                                              Pluto's past, present and future orientation is controll
103 nt of gaseous methane a few kilometres above Pluto's plains that favours methane condensation at moun
104  a positive gravity signature that locks, as Pluto's rotation slows, to a longitude directly opposite
105                                              Pluto's Sputnik Planitia is a bright, roughly circular f
106                                              Pluto's surface displays diverse landforms, terrain ages
107                                              Pluto's surface exhibits complex regional color diversit
108                           Similar colours on Pluto's surface have been attributed to tholin-like orga
109 on monoxide, and nitrogen ices that dominate Pluto's surface have complicated spatial distributions r
110                                              Pluto's surface is surprisingly young and geologically a
111 pheric hazes, rather than gases, can explain Pluto's temperature profile.
112 been proposed as a coolant; however, because Pluto's thermal structure is expected to be in radiative
113 a, is located very close to the longitude of Pluto's tidal axis and may be an impact feature, by anal
114 nformally named Sputnik Planum is central to Pluto's vigorous geological activity.
115                                              Pluto's water ice "bedrock" was also mapped, with isolat
116 e than a few tens of metres, consistent with Pluto's youngest terrains.
117                   Its surface is darker than Pluto's, suggesting that it is largely devoid of fresh i
118 es of the southern hemisphere illuminated by Pluto-shine and also images taken during the approach ph
119 ter and there are no fundamental reasons why Pluto should not have more satellites.
120  on similarly sized KBOs that do not orbit a Pluto-sized object to draw an escaping atmosphere from,
121  compositional data showing that terrains on Pluto span a variety of ages, ranging from relatively an
122                        The Solar Wind Around Pluto (SWAP) instrument revealed an interaction region c
123                                          The Pluto system was recently explored by NASA's New Horizon
124 able optical depths form sporadically in the Pluto system, and that rich satellite systems may be fou
125 6 kilometers(-3) for the dust density in the Pluto system.
126 egrees, almost directly opposite the side of Pluto that always faces Charon as a result of tidal lock
127                                     Gas from Pluto that is transiently cold-trapped and processed at
128 ) and S/2005 P 2 (hereafter P2), which makes Pluto the first Kuiper belt object known to have multipl
129                                              Pluto, Titan, and Triton make up a unique class of solar
130 ed an interaction region confined sunward of Pluto to within about 6 Pluto radii.
131                                              PLUTO transports uracil, adenine, and guanine with appar
132  since the first member object, not counting Pluto, was discovered in 1992.
133 ed, Charon raises a permanent tidal bulge on Pluto, which greatly enhances the gravity signature of t
134  (approximately 1,200 km) about half that of Pluto, which makes it larger, relative to its primary, t
135 Charon is found to be different from that of Pluto, with water ice in crystalline form covering most

 
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