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1 tion slows, to a longitude directly opposite Charon.
2 as revealed the complex geology of Pluto and Charon.
3 cause of the permanent tidal bulge raised by Charon.
4 on tidal axis, on the far side of Pluto from Charon.
5 l to the common pole directions of Pluto and Charon.
6 ydra have bright surfaces similar to that of Charon.
7 planet' comprising Pluto and its large moon, Charon.
8 for producing the observed colour pattern on Charon.
9  orbits exterior to Pluto's large satellite, Charon.
10 g as debris from the collision that produced Charon.
11 ion observations of a stellar occultation by Charon.
12 st known members are Pluto and its companion Charon.
13 lving a trans-Neptunian satellite other than Charon.
14 cross the encounter hemispheres of Pluto and Charon.
15 to genomic library packaged in bacteriophage charon 35.
16 in the same plane as Pluto's large satellite Charon, along with their apparent locations in or near h
17 t such an impact probably produced an intact Charon, although it is possible that a disk of material
18  We model the surface thermal environment on Charon and the supply and temporary cold-trapping of mat
19       Impact crater populations on Pluto and Charon are not consistent with the steepest impactor siz
20                          Pluto and its moon, Charon, are the most prominent members of the Kuiper bel
21 symmetric expression of the Nodal antagonist charon around the KV and show that Nkd1 knockdown impact
22 opposite the side of Pluto that always faces Charon as a result of tidal locking.
23      Taken together, these results implicate Charon as an essential mediator of PARP-1-dependent tran
24 ly, driven by the large torques of the Pluto-Charon binary.
25 rmath of a collision that produced the Pluto-Charon binary.
26 d to demonstrate that the formation of Pluto-Charon by means of a large collision is quite plausible.
27  a genetically encoded fluorescent reporter, CharON (Caspase and pH Activated Reporter, Fluorescence
28 on, normal expression of southpaw (spaw) and charon (cha) in the peri-KV region and normal expression
29 , the method relies on the combined use of a CHARON ("Chemical Analysis of Aerosol Online") particle
30 s that Sputnik Planitia formed shortly after Charon did and has been stable, albeit gradually losing
31                           Pluto's large moon Charon displays tectonics and evidence for a heterogeneo
32                                              Charon does not appear to be currently active, but exper
33 driven outward by resonant interactions with Charon during its tidal orbital expansion.
34 tical to situs solitus via robust asymmetric charon expression.
35  show that Nkd1 knockdown impacts asymmetric charon expression.
36 sional ejecta that originated from the Pluto-Charon formation event.
37                      It has been argued that Charon formed as a result of a giant impact with primord
38     Observations have resolved the satellite Charon from its parent planet Pluto, giving separate spe
39 that a previously unknown protein, termed as Charon, functions as a regulator of antibacterial and an
40                        The polar location on Charon implicates the temperature extremes that result f
41  The observation of a stellar occultation by Charon in 1980 established a lower limit on its radius o
42 g the "Chemical Analysis of Aerosol Online" (CHARON) inlet.
43                 Our results demonstrate that Charon interacts with the NF-kappaB ortholog Relish insi
44  and antifungal immune defense in Drosophila Charon is an ankyrin repeat-containing protein that medi
45                              The spectrum of Charon is found to be different from that of Pluto, with
46  A unique feature of Pluto's large satellite Charon is its dark red northern polar cap.
47  a disk of material orbited Pluto from which Charon later accumulated.
48                The existence of such ices on Charon may indicate geological activity in the satellite
49 ristics, including ones similar to the Pluto-Charon pair.
50                                              Charon, Pluto's largest moon, has been extensively studi
51                   Ablating the expression of Charon prevents Relish from targeting promoters of antim
52 sical characteristics of Pluto and its moon, Charon, provide insight into the evolution of the outer
53 f carbon vs carbon number) revealed that the CHARON-PTR-ToF-MS technique adds significant analytical
54                                 Once locked, Charon raises a permanent tidal bulge on Pluto, which gr
55                                              Charon's color pattern is simpler, dominated by neutral
56                    Within a million years of Charon's formation, ice deposits on Pluto concentrate in
57 es the temperature extremes that result from Charon's high obliquity and long seasons in the producti
58 e show an endogenic source of volatiles from Charon's interior is plausible.
59 ss, and between 5 x 10(-3) and 1 x 10(-4) of Charon's mass.
60                                              Charon's near-infrared spectra reveal highly localized a
61  dark coloration on the basis of an image of Charon's northern hemisphere, but not modelled quantitat
62 drogen peroxide (H(2)O(2)) on the surface of Charon's northern hemisphere, using JWST data.
63         This could have been accomplished if Charon's orbit was eccentric during most of this orbital
64                  Previous work proposed that Charon's organic-rich north pole formed from radiolytica
65 wo new moons are nearly integer multiples of Charon's period, suggesting that they were driven outwar
66 controls the distribution and composition of Charon's photoproducts.
67 is volcanically released methane migrates to Charon's poles, with deposition rates sufficient to be p
68        In addition, an absorption feature in Charon's spectrum suggests the presence of ammonia ices.
69 1.29 x 10(15)-3.47 x 10(15) kg of methane to Charon's surface from its interior.
70 is transiently cold-trapped and processed at Charon's winter pole was proposed as an explanation for
71                                  Our initial CHARON studies did not take into account fragmentation o
72 s, and the New Horizons mission to the Pluto-Charon system allows us to test hypotheses on the origin
73 ent with collisional formation for the Pluto-Charon system in which the precursor objects may have be
74 out 570 days), very different from the Pluto/Charon system, which was hitherto the only previously kn
75 ates a photolytic refractory distribution on Charon that increases with latitude, consistent with pol
76 es that are small compared to both Pluto and Charon-that is, between 5 x 10(-4) and 1 x 10(-5) of Plu
77 show that P1 and P2's proximity to Pluto and Charon, the fact that P1 and P2 are on near-circular orb
78 uld have moved the feature towards the Pluto-Charon tidal axis, on the far side of Pluto from Charon.
79    This large feature is very near the Pluto-Charon tidal axis.
80               Pluto's first known satellite, Charon, was discovered in 1978.
81                  Using Drosophila expressing CharON, we uncovered multiple qualitative and quantitati
82   These new satellites are much smaller than Charon, with estimates of P1's diameter ranging from 60
83 circular orbits in the same orbital plane as Charon, with orbital periods of approximately 38 days (P