ライフサイエンスコーパス: Pluto

1 proximately 40 per cent greater than that of Pluto).

2 as a result of volatile transport cycles on Pluto.

3 uction of an extensive haze that encompasses Pluto.

4 stimated present-day heat-flow conditions on Pluto.

5 ely replicate the observed fault networks on Pluto.

6 sulting reorientation (true polar wander) of Pluto.

7 x 10(22) kilograms, or 1.27 +/- 0.02 that of Pluto.

8 s a result of a giant impact with primordial Pluto.

9 ions are accelerated and/or deflected around Pluto.

10 s spacecraft in the Tartarus Dorsa region of Pluto (220 degrees -250 degrees E, 0 degrees -20 degrees

11 Pluto also has ancient cratered terrains up to ~4 billio

12 Impact crater populations on Pluto and Charon are not consistent with the steepest im

13 Here we show that P1 and P2's proximity to Pluto and Charon, the fact that P1 and P2 are on near-ci

14 have masses that are small compared to both Pluto and Charon-that is, between 5 x 10(-4) and 1 x 10(

15 spectra across the encounter hemispheres of Pluto and Charon.

16 acecraft has revealed the complex geology of Pluto and Charon.

17 orthogonal to the common pole directions of Pluto and Charon.

18 Triton is as large as Pluto and is postulated to have been captured from helio

19 eyond Neptune; the largest known members are Pluto and its companion Charon.

20 round the central 'binary planet' comprising Pluto and its large moon, Charon.

21 Pluto and its moon, Charon, are the most prominent membe

22 The physical characteristics of Pluto and its moon, Charon, provide insight into the evo

23 ore distant satellites of Pluto, reveal that Pluto and its moons comprise an unusual, highly compact,

24 near the same wavelengths in the spectra of Pluto and Neptune's satellite Triton are due to CH4 on t

25 ain N-bearing molecule in the atmospheres of Pluto and Triton and probably the main nitrogen reservoi

26 nts that measured the space environment near Pluto as it flew by on 14 July 2015.

27 rary cold-trapping of material escaping from Pluto, as well as the photolytic processing of this mate

28 other solar nebula bodies such as Triton and Pluto, but is very different from that of the regular sa

29 e aftermath of a collision that produced the Pluto-Charon binary.

30 otically, driven by the large torques of the Pluto-Charon binary.

31 re used to demonstrate that the formation of Pluto-Charon by means of a large collision is quite plau

32 collisional ejecta that originated from the Pluto-Charon formation event.

33 aracteristics, including ones similar to the Pluto-Charon pair.

34 onsistent with collisional formation for the Pluto-Charon system in which the precursor objects may h

35 der could have moved the feature towards the Pluto-Charon tidal axis, on the far side of Pluto from C

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

37 od (about 570 days), very different from the Pluto/Charon system, which was hitherto the only previou

38 years of Charon's formation, ice deposits on Pluto concentrate into a single cap centred near a latit

39 Observations from the Pluto Energetic Particle Spectrometer Science Investigat

40 PLUTO (for plastidic nucleobase transporter) was identif

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

42 is possible that a disk of material orbited Pluto from which Charon later accumulated.

43 tions of a proton uncoupler, indicating that PLUTO functions as a proton-substrate symporter.

44 the satellite Charon from its parent planet Pluto, giving separate spectra of the two objects from 1

45 A PLUTO green fluorescent protein fusion was shown to resi

46 Two small moons of Pluto have been discovered in low-eccentricity orbits ex

47 revious searches for other satellites around Pluto have been unsuccessful, but they were not sensitiv

48 Heterologous expression of PLUTO in an Escherichia coli mutant lacking the bacteria

49 d wavelengths of an occultation of a star by Pluto in August 2002.

50 on a recent model representing conditions on Pluto, in which deepening penitentes reproduce both the

51 The deep nitrogen-covered basin on Pluto, informally named Sputnik Planitia, is located ver

52 Pluto is an astoundingly diverse, geologically dynamic w

53 We predict that Pluto is therefore several orders of magnitude brighter

54 g that shows that ice quickly accumulates on Pluto near latitudes of 30 degrees north and south, even

55 N2 are inconsistent with the observations on Pluto of non-brittle deformation within the N2-ice sheet

56 The two newly discovered satellites of Pluto (P1 and P2) have masses that are small compared to

57 indeed form as a result of an impact and if Pluto possesses a subsurface ocean, the required positiv

58 the discovery of two additional moons around Pluto, provisionally designated S/2005 P 1 (hereafter P1

59 confined sunward of Pluto to within about 6 Pluto radii.

60 on the absence of more distant satellites of Pluto, reveal that Pluto and its moons comprise an unusu

61 These data reveal evidence for extinction in Pluto's atmosphere and show that it has indeed changed,

62 Occultation data acquired for Pluto's atmosphere in 1988 revealed a nearly isothermal

63 Pluto's atmosphere is cold and hazy.

64 Pluto's atmosphere is highly extended, with trace hydroc

65 It is unclear whether the current state of Pluto's atmosphere is representative of its average stat

66 We conclude that Pluto's atmosphere is unique among Solar System planetar

67 Another question is to what extent Pluto's atmosphere might be collapsing as it recedes fro

68 The escape of Pluto's atmosphere provides a potential feedstock for a

69 enhanced-Jeans, hydrodynamic-like escape of Pluto's atmosphere to space.

70 a detailed snapshot of the current state of Pluto's atmosphere.

71 averaged over its orbital period, those are Pluto's coldest regions.

72 Pluto's diverse surface geology and long-term activity r

73 Pluto's encounter hemisphere shows ongoing surface geolo

74 Pluto's first known satellite, Charon, was discovered in

75 of Sputnik Planitia can substantially alter Pluto's inertia tensor, resulting in a reorientation of

76 ensation, changing insolation conditions and Pluto's interior structure.

77 Pluto's large moon Charon displays tectonics and evidenc

78 A unique feature of Pluto's large satellite Charon is its dark red northern

79 on near-circular orbits in the same plane as Pluto's large satellite Charon, along with their apparen

80 vered in low-eccentricity orbits exterior to Pluto's large satellite, Charon.

81 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

82 ission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra.

83 Pluto's past, present and future orientation is controll

84 a positive gravity signature that locks, as Pluto's rotation slows, to a longitude directly opposite

85 Pluto's Sputnik Planitia is a bright, roughly circular f

86 Pluto's surface displays diverse landforms, terrain ages

87 Pluto's surface exhibits complex regional color diversit

88 Similar colours on Pluto's surface have been attributed to tholin-like orga

89 on monoxide, and nitrogen ices that dominate Pluto's surface have complicated spatial distributions r

90 Pluto's surface is surprisingly young and geologically a

91 pheric hazes, rather than gases, can explain Pluto's temperature profile.

92 been proposed as a coolant; however, because Pluto's thermal structure is expected to be in radiative

93 a, is located very close to the longitude of Pluto's tidal axis and may be an impact feature, by anal

94 nformally named Sputnik Planum is central to Pluto's vigorous geological activity.

95 Pluto's water ice "bedrock" was also mapped, with isolat

96 e than a few tens of metres, consistent with Pluto's youngest terrains.

97 Its surface is darker than Pluto's, suggesting that it is largely devoid of fresh i

98 es of the southern hemisphere illuminated by Pluto-shine and also images taken during the approach ph

99 ter and there are no fundamental reasons why Pluto should not have more satellites.

100 The Solar Wind Around Pluto (SWAP) instrument revealed an interaction region c

101 The Pluto system was recently explored by NASA's New Horizon

102 able optical depths form sporadically in the Pluto system, and that rich satellite systems may be fou

103 6 kilometers(-3) for the dust density in the Pluto system.

104 egrees, almost directly opposite the side of Pluto that always faces Charon as a result of tidal lock

105 Gas from Pluto that is transiently cold-trapped and processed at

106 ) and S/2005 P 2 (hereafter P2), which makes Pluto the first Kuiper belt object known to have multipl

107 ed an interaction region confined sunward of Pluto to within about 6 Pluto radii.

108 PLUTO transports uracil, adenine, and guanine with appar

109 since the first member object, not counting Pluto, was discovered in 1992.

110 ed, Charon raises a permanent tidal bulge on Pluto, which greatly enhances the gravity signature of t

111 (approximately 1,200 km) about half that of Pluto, which makes it larger, relative to its primary, t

112 Charon is found to be different from that of Pluto, with water ice in crystalline form covering most