ライフサイエンスコーパス: Charon

1 as revealed the complex geology of Pluto and Charon.

2 cause of the permanent tidal bulge raised by Charon.

3 on tidal axis, on the far side of Pluto from Charon.

4 for producing the observed colour pattern on 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 orbits exterior to Pluto's large satellite, Charon.

9 g as debris from the collision that produced Charon.

10 ion observations of a stellar occultation by Charon.

11 st known members are Pluto and its companion Charon.

12 cross the encounter hemispheres of Pluto and Charon.

13 tion slows, to a longitude directly opposite Charon.

14 to genomic library packaged in bacteriophage charon 35.

15 in the same plane as Pluto's large satellite Charon, along with their apparent locations in or near h

16 t such an impact probably produced an intact Charon, although it is possible that a disk of material

17 We model the surface thermal environment on Charon and the supply and temporary cold-trapping of mat

18 Impact crater populations on Pluto and Charon are not consistent with the steepest impactor siz

19 Pluto and its moon, Charon, are the most prominent members of the Kuiper bel

20 symmetric expression of the Nodal antagonist charon around the KV and show that Nkd1 knockdown impact

21 opposite the side of Pluto that always faces Charon as a result of tidal locking.

22 Taken together, these results implicate Charon as an essential mediator of PARP-1-dependent tran

23 ly, driven by the large torques of the Pluto-Charon binary.

24 rmath of a collision that produced the Pluto-Charon binary.

25 d to demonstrate that the formation of Pluto-Charon by means of a large collision is quite plausible.

26 on, normal expression of southpaw (spaw) and charon (cha) in the peri-KV region and normal expression

27 , the method relies on the combined use of a CHARON ("Chemical Analysis of Aerosol Online") particle

28 s that Sputnik Planitia formed shortly after Charon did and has been stable, albeit gradually losing

29 Pluto's large moon Charon displays tectonics and evidence for a heterogeneo

30 Charon does not appear to be currently active, but exper

31 driven outward by resonant interactions with Charon during its tidal orbital expansion.

32 tical to situs solitus via robust asymmetric charon expression.

33 show that Nkd1 knockdown impacts asymmetric charon expression.

34 sional ejecta that originated from the Pluto-Charon formation event.

35 It has been argued that Charon formed as a result of a giant impact with primord

36 Observations have resolved the satellite Charon from its parent planet Pluto, giving separate spe

37 that a previously unknown protein, termed as Charon, functions as a regulator of antibacterial and an

38 The polar location on Charon implicates the temperature extremes that result f

39 The observation of a stellar occultation by Charon in 1980 established a lower limit on its radius o

40 Our results demonstrate that Charon interacts with the NF-kappaB ortholog Relish insi

41 and antifungal immune defense in Drosophila Charon is an ankyrin repeat-containing protein that medi

42 The spectrum of Charon is found to be different from that of Pluto, with

43 A unique feature of Pluto's large satellite Charon is its dark red northern polar cap.

44 a disk of material orbited Pluto from which Charon later accumulated.

45 The existence of such ices on Charon may indicate geological activity in the satellite

46 ristics, including ones similar to the Pluto-Charon pair.

47 Ablating the expression of Charon prevents Relish from targeting promoters of antim

48 sical characteristics of Pluto and its moon, Charon, provide insight into the evolution of the outer

49 f carbon vs carbon number) revealed that the CHARON-PTR-ToF-MS technique adds significant analytical

50 Once locked, Charon raises a permanent tidal bulge on Pluto, which gr

51 Charon's color pattern is simpler, dominated by neutral

52 Within a million years of Charon's formation, ice deposits on Pluto concentrate in

53 es the temperature extremes that result from Charon's high obliquity and long seasons in the producti

54 ss, and between 5 x 10(-3) and 1 x 10(-4) of Charon's mass.

55 Charon's near-infrared spectra reveal highly localized a

56 dark coloration on the basis of an image of Charon's northern hemisphere, but not modelled quantitat

57 This could have been accomplished if Charon's orbit was eccentric during most of this orbital

58 wo new moons are nearly integer multiples of Charon's period, suggesting that they were driven outwar

59 In addition, an absorption feature in Charon's spectrum suggests the presence of ammonia ices.

60 is transiently cold-trapped and processed at Charon's winter pole was proposed as an explanation for

61 ent with collisional formation for the Pluto-Charon system in which the precursor objects may have be

62 out 570 days), very different from the Pluto/Charon system, which was hitherto the only previously kn

63 es that are small compared to both Pluto and Charon-that is, between 5 x 10(-4) and 1 x 10(-5) of Plu

64 show that P1 and P2's proximity to Pluto and Charon, the fact that P1 and P2 are on near-circular orb

65 uld have moved the feature towards the Pluto-Charon tidal axis, on the far side of Pluto from Charon.

66 This large feature is very near the Pluto-Charon tidal axis.

67 Pluto's first known satellite, Charon, was discovered in 1978.

68 These new satellites are much smaller than Charon, with estimates of P1's diameter ranging from 60

69 circular orbits in the same orbital plane as Charon, with orbital periods of approximately 38 days (P