ライフサイエンスコーパス: Jupiter

1 = 57.0 days) with a mass 0.37 times that of Jupiter.

2 ing the planets and forming a retrograde hot Jupiter.

3 isotopic composition is the same as that of Jupiter.

4 dies in orbit about the Sun between Mars and Jupiter.

5 nterior of Saturn, and to a lesser extent in Jupiter.

6 he Earth's atmosphere has been discovered in Jupiter.

7 retrograde co-orbital asteroid of the planet Jupiter.

8 enomenon similar to that on the Earth and in Jupiter.

9 ith mass no greater than a few times that of Jupiter.

10 n contrast to a recent claim for another hot Jupiter.

11 her latitudes flow both east and west, as on Jupiter.

12 seasonal scales at mid- and low latitudes on Jupiter.

13 ers and resonances with one another and with Jupiter.

14 4.617 days and a mass at least 0.69 that of Jupiter.

15 l influence of the newly formed giant planet Jupiter.

16 ays and a minimum mass of 1.14 times that of Jupiter.

17 morphologically from those of both Earth and Jupiter.

18 m, possibly not at its present location near Jupiter.

19 tering of precursor objects after capture by Jupiter.

20 core-accretion process that may have formed Jupiter.

21 ative energy balance on other planets, as on Jupiter.

22 l energy balance in the middle atmosphere of Jupiter.

23 rmation models indicate a mass twice that of Jupiter.

24 th masses similar to or greater than that of Jupiter.

25 n migration as a mechanism for producing hot Jupiters.

26 System, and contrasts with the isolated hot Jupiters.

27 ons would be implicated as the origin of hot Jupiters.

28 monoxide (CO) have been detected in two hot Jupiters.

29 ms occur with a frequency similar to the hot Jupiters.

30 te a major channel for the production of hot Jupiters.

31 chaos and applying it to Mercury and to hot Jupiters.

32 Intervention Trial Evaluating Rosuvastatin (JUPITER), 17 802 apparently healthy men and women with l

33 planet's mass is at most three times that of Jupiter; a higher mass would lead to gravitational disru

34 seen from individual volcanoes near Io's sub-Jupiter and anti-Jupiter points.

35 ontrolled trials of both primary prevention (JUPITER and ASCOT) and secondary prevention (CARE and PR

36 st to planets with masses similar to that of Jupiter and higher, the bulk compositions of planets in

37 A strong interaction between Jupiter and its plasma environment produces hot spots in

38 emissions associated with the interaction of Jupiter and its satellite Io extend to a surprisingly hi

39 rms of asteroids following the same orbit as Jupiter and located at the L4 and L5 stable Lagrange poi

40 of small objects orbiting primarily between Jupiter and Neptune--with an equivalent radius of 124 +/

41 .71 and approximately 0.27 times the mass of Jupiter and orbital separations of approximately 2.3 and

42 Retrograde co-orbital asteroids of Jupiter and other planets may be more common than previo

43 itational resonances during the migration of Jupiter and Saturn approximately 4 Gyr ago.

44 y when the orbital effects of large planets (Jupiter and Saturn) and damping mechanisms, such as gas

45 the cloud into scattered patches (as seen on Jupiter and Saturn).

46 itu dust instruments around the icy moons of Jupiter and Saturn, but have hitherto not been observed

47 ion on other icy bodies such as the moons of Jupiter and Saturn, has remained undetected in cometary

48 h show that a popular formation scenario for Jupiter and Saturn, in which Jupiter migrates inward fro

49 al differences between the magnetospheres of Jupiter and Saturn, it has been suggested that cryovolca

50 to be important for particle acceleration at Jupiter and Saturn, the electric field produced in the i

51 t step in forming gas-giant planets, such as Jupiter and Saturn, was the production of solid 'cores'

52 Unlike on the icy satellites of Jupiter and Saturn, where tidal forces are responsible f

53 destroyed the picture--established by Earth, Jupiter and Saturn--that planetary magnetic fields are d

54 tures of the planets are similar to those of Jupiter and Saturn.

55 earch for microbial life on the icy moons of Jupiter and Saturn.

56 planets, but nearly all are gas giants like Jupiter and Saturn.

57 lination distributions of irregular moons at Jupiter and Saturn.

58 depletion caused by the orbital migration of Jupiter and Saturn.

59 rents of a different nature were observed at Jupiter and their presence inferred at Saturn.

60 These differences between hot Jupiters and other planetary systems denote a distinctly

61 Intervention Trial Evaluating Rosuvastatin (JUPITER) and performed replication in a meta-analysis of

62 Intervention Trial Evaluating Rosuvastatin (JUPITER) and synthesized the results with prior trials.

63 isk, and 25 in those at high genetic risk in JUPITER, and 57, 47, and 20, respectively, in ASCOT.

64 the planetary mass at four times the mass of Jupiter, and constrains the planet's tidal luminosity.

65 rther stratify risk in patients eligible for JUPITER, and could be used to target subgroups of patien

66 red during cruise phase outside the orbit of Jupiter, and find a statistical upper limit on the optic

67 explanation for the high obliquities of hot Jupiters, and dynamical interactions would be implicated

68 gration that produces warm Jupiters over hot Jupiters, and they provide evidence for a population of

69 een in the auroral emissions from Saturn and Jupiter are due to scaling differences in the conditions

70 Hot Jupiters are gas-giant planets orbiting with periods of

71 Many exoplanetary systems containing hot Jupiters are observed to have highly misaligned orbital

72 Stars hosting hot Jupiters are often observed to have high obliquities, wh

73 revealed that a considerable fraction of hot Jupiters are on orbits that are misaligned with respect

74 Close-in giant planets (e.g., "hot Jupiters") are thought to form far from their host stars

75 The atmospheres of these 'hot Jupiters' are heated by the immense stellar irradiation.

76 Indeed, isolated 'hot Jupiters' are often misaligned and even orbiting retrogr

77 edictions for the most highly irradiated hot-Jupiter atmospheres.

78 Among such intermediate-risk patients, a JUPITER-based strategy becomes cost-saving at a rosuvast

79 In JUPITER, baseline LDL-C was not associated with CVD even

80 oid belt lies between the orbits of Mars and Jupiter, but the region is not uniformly filled with ast

81 oscillations (with a 4-5-yr cycle) occur on Jupiter, but these data suffer from poor vertical resolu

82 he Jupiter-Sun system (leading and following Jupiter by 60 degrees ).

83 itors being more efficiently swept away from Jupiter by its galilean moons.

84 e orbits lie close to their host stars ('hot Jupiters') can largely be accounted for by planetary mig

85 In JUPITER, cholesterol efflux capacity was associated with

86 The hot Jupiters closest to their parent stars, at orbital dista

87 rticular, we predict that liquid iron in the Jupiter core is in the "rigid liquid" state and is highl

88 A hot Jupiter could be the end state of a secularly chaotic pl

89 ligned electron beams associated with the Io-Jupiter coupling, for example, create an auroral footpri

90 results from a comparative study of ten hot Jupiters covering the wavelength range 0.3-5 micrometres

91 (JUPITER-Crestor 20 mg Versus Placebo in Prevention of Ca

92 (JUPITER-Crestor 20mg Versus Placebo in Prevention of Car

93 JUPITER demonstrated that in primary prevention rosuvast

94 In images taken in Jupiter eclipse, nonthermal visible-wavelength emission

95 2.6 million women age > or =60 years meeting JUPITER eligibility criteria had fasting LDL-C <130 mg/d

96 Extrapolating JUPITER eligibility to NHANES, an estimated 6.5 million

97 ligible participants, 18.2% (n = 1,621) were JUPITER-eligible (hs-CRP > or = 2.0 mg/l, LDL-C <130 mg/

98 Rosuvastatin treatment for JUPITER-eligible patients appears to be cost-effective,

99 this study is to describe the proportion of "JUPITER-eligible" (Justification for the Use of statins

100 Atheroslcerosis (MESA) met all criteria for JUPITER entry.

101 e equivalent (including diabetes), and other JUPITER exclusions.

102 with observations and in studies of the hot Jupiter exoplanet HD 189733b leads to up to a 20-fold in

103 Recent studies show that some hot-Jupiter exoplanets have much weaker water absorption fea

104 'Hot Jupiter' extrasolar planets are expected to be tidally l

105 rared observations of more than a dozen 'hot-Jupiter' extrasolar planets have now been reported.

106 About 25 per cent of 'hot Jupiters' (extrasolar Jovian-mass planets with close-in

107 rge gaps in compositional maps of Ganymede's Jupiter-facing hemisphere.

108 in situ measurement of the D/H ratio in the Jupiter family comet 67P/Churyumov-Gerasimenko by the RO

109 the direct in situ measurement of N2 in the Jupiter family comet 67P/Churyumov-Gerasimenko, made by

110 wide range of D/H ratios in the water within Jupiter family objects and preclude the idea that this r

111 HCN, CO, CH3OH, H2CO, C2H2, and CH4) in the Jupiter-family comet Tempel 1 using high-dispersion infr

112 rs per second from an orbit close to that of Jupiter-family comets (Tisserand's parameter = 2.8 +/- 0

113 The JUPITER findings are supported by two recent meta-analys

114 Of these locations, Jupiter Florida/Vero Beach has the highest settlement ra

115 ly given the inputs and limits of the model; Jupiter Florida/Vero Beach, the Cape Hatteras Tropical L

116 is has been interpreted as evidence that hot-Jupiter formation is linked to dynamical disruption, as

117 ovided the motivation for our meta-analysis (JUPITER) had little impact on the findings for venous th

118 has only one large satellite, Titan, whereas Jupiter has four large satellites; additional large sate

119 However, radiative forcing on Jupiter has traditionally been attributed to solar heati

120 Europa, the innermost icy satellite of Jupiter, has a tortured young surface and sustains a liq

121 ng outer ice shell about the tidal axis with Jupiter, has been proposed as a possible explanation for

122 If JUPITER hazard ratios were applied to this group, the nu

123 ement between the mass retrieved for the hot Jupiter HD 189733b from transmission spectroscopy with t

124 Intervention Trial Evaluating Rosuvastatin (JUPITER), HDL size and HDL-P were measured by nuclear ma

125 ity are similar to variations seen closer to Jupiter in Galileo data.

126 The Composite Infrared Spectrometer observed Jupiter in the thermal infrared during the swing-by of t

127 l friction, and find that we can produce hot Jupiters in orbits that are retrograde with respect to t

128 distinct from those of the icy satellites of Jupiter, in both brightness and polarization.

129 tion in the deep metallic hydrogen region of Jupiter is believed to generate its magnetic field, the

130 Because Jupiter is closer than the other giant planets, searches

131 actions with the solar wind, whereas that at Jupiter is formed through interactions with plasma from

132 Dust near Jupiter is produced when interplanetary impactors collid

133 Thus, Jupiter is the oldest planet of the Solar System, and it

134 on regions dominate: the upper atmosphere of Jupiter itself, and a torus of emission residing just ou

135 cipants in the randomized placebo-controlled JUPITER (Justification for the Use of Statins in Prevent

136 vastatin in apparently healthy adults in the JUPITER (Justification for the Use of Statins in Prevent

137 luate the cost-effectiveness of applying the JUPITER (Justification for the Use of statins in Prevent

138 Within the JUPITER (Justification for the Use of statins in Prevent

139 or patients with a proinflammatory response, JUPITER (Justification for the Use of Statins in Prevent

140 Rosuvastatin therapy in the JUPITER (Justification for the Use of Statins in Primary

141 rdiac Outcomes Trial-Lipid-Lowering Arm] and JUPITER [Justification for the Use of Statins in Prevent

142 ency (=0.02), and randomized clinical trial (JUPITER [Justification for the Use of Statins in Primary

143 ric stability between 0.14 and 0.16 au for a Jupiter-like planet orbiting a solar-type star.

144 guration of these planets, combined with the Jupiter-like size of their host star-named TRAPPIST-1-ma

145 ightness of the host star, combined with its Jupiter-like size, offers the possibility of thoroughly

146 gnetosphere was reduced, resulting in a more Jupiter-like system, in agreement with the dearth of aur

147 95 per cent upper limit on the frequency of Jupiter-mass free-floating or wide-orbit planets of 0.25

148 a large population of unbound or wide-orbit Jupiter-mass planets (reported to be almost twice as com

149 could limit the largest moons of extrasolar Jupiter-mass planets to Moon-to-Mars size.

150 rbital period of 0.94 days and a mass of ten Jupiter masses (10 M(Jup)), resulting in a tidal interac

151 probably induced by an object of around 0.9 Jupiter masses in an orbit only 0.023 au from its star.

152 131399Ab is one of the lowest mass (4 +/- 1 Jupiter masses) and coldest (850 +/- 50 kelvin) exoplane

153 tudies are incomplete for objects below five Jupiter masses.

154 on scenario for Jupiter and Saturn, in which Jupiter migrates inward from a > 5 astronomical units (A

155 his efficient separation is the formation of Jupiter, opening a gap in the disk and preventing the ex

156 extrasolar giant planets--the so-called 'hot Jupiters'--orbit within 0.05 au of their primary stars (

157 ere I report the detection of an unusual hot Jupiter orbiting the primary star of a triple stellar sy

158 ersion of tidal migration that produces warm Jupiters over hot Jupiters, and they provide evidence fo

159 n Ceres, the largest object between Mars and Jupiter, over the last 4.55 Gyr.

160 JUPITER participants included 6801 women > or =60 years

161 Among white JUPITER participants treated with potent statin therapy,

162 ith those with eGFR >or=60 ml/min/1.73 m(2), JUPITER participants with moderate CKD had higher vascul

163 h CRP reduction among 3380 placebo-allocated JUPITER participants.

164 Intervention Trial Evaluating Rosuvastatin (JUPITER) participants, we tested whether lipids, apolipo

165 spacecraft acquired science observations of Jupiter, passing less than 5000 kilometers above the equ

166 h for planetary companions orbiting near hot Jupiter planet candidates (Jupiter-size candidates with

167 etection of TiO in the atmosphere of the hot-Jupiter planet WASP-19b.

168 in space exploration missions (i.e., Venus &Jupiter planetary exploration, and heliophysics missions

169 o be abundant in the upper atmosphere of hot-Jupiter planets, but is not identifiable here; therefore

170 mary sources of non-continuum opacity in hot-Jupiter planets.

171 Models of these 'hot Jupiter' planets predict a flux peak near 10 microm, whe

172 Yet models of such 'hot-Jupiter' planets predict an abundance of atmospheric wat

173 ual volcanoes near Io's sub-Jupiter and anti-Jupiter points.

174 ng has been seen on other planets, including Jupiter, polar lightning has been known only on Earth.

175 444 (47%) patients in the MESA JUPITER population had CAC scores of 0 and, in this grou

176 association between these quartiles and the JUPITER primary endpoint of first non-fatal myocardial i

177 INTERPRETATION: In the JUPITER primary prevention trial, the cardiovascular and

178 meta-analysis across the WOSCOPS, ASCOT, and JUPITER primary prevention, relative risk reduction in t

179 w exoplanets with sizes between 0.37 and 1.6 Jupiter radii and orbital periods from 3.2 to 4.9 days w

180 o, a giant nebula extending out to about 500 Jupiter radii, and a jet close to Io.

181 of the hot Jupiter, the innermost planet was Jupiter (rather than Mercury) sized, and its chaotic evo

182 intervention Trial Evaluating Rosuvastatin (JUPITER) reignited attention on the link between statin

183 d spectral measurements over five successive Jupiter rotations at spatial resolutions of 200 to 140 k

184 Radio wavelengths can probe altitudes in Jupiter's atmosphere below its visible cloud layers.

185 Jupiter's atmosphere is stable, so somewhere between 5 a

186 Several observations of Jupiter's atmosphere made by instruments on the New Hori

187 Jupiter's atmosphere, as observed in the 1979 Voyager sp

188 downward, discrete electron acceleration in Jupiter's auroral polar regions.

189 However, preliminary in situ measurements of Jupiter's auroral regions yielded no evidence of such a

190 As such, our results indicate that Jupiter's core grew to approximately 20 Earth masses wit

191 nterior, including the existence and mass of Jupiter's core.

192 quatorial wave, bringing up ammonia gas from Jupiter's deep atmosphere.

193 ximately 2 x 10(-8) is comparable to that of Jupiter's faintest gossamer ring, although its particle

194 The best known exceptions are Jupiter's gossamer rings and Saturn's E ring, broad shee

195 pirals, each winding up at a rate defined by Jupiter's gravity field.

196 uno's passage over the poles and traverse of Jupiter's hazardous inner radiation belts.

197 he comparatively sparse crater population on Jupiter's icy moon Europa and suggest that this assumpti

198 The New Horizons spacecraft observed Jupiter's icy satellites Europa and Ganymede during its

199 Amalthea and Thebe may be the remnants of Jupiter's inflowing building blocks that formed in the o

200 Jupiter's inward migration entrained s greater, similar

201 plasmoids-and contains ions from both Io and Jupiter's ionosphere with intense bursts of H(+) and H(+

202 for example, create an auroral footprint in Jupiter's ionosphere.

203 When the solar wind hits Jupiter's magnetic field, it creates a long magnetotail

204 and the barely understood electron beams in Jupiter's magnetosphere, demonstrate that anti-planetwar

205 port the analysis of 50-80 keV ENA images of Jupiter's magnetosphere, where two distinct emission reg

206 conclusively demonstrated by observations in Jupiter's magnetosphere, which--like that of Saturn (but

207 umes on Io's electrodynamic interaction with Jupiter's magnetosphere.

208 ssible source region along the dusk flank of Jupiter's magnetosphere.

209 to Io's atmosphere and its interaction with Jupiter's magnetosphere.

210 he structure of, and the energy flow within, Jupiter's magnetosphere.

211 Jupiter's magnetospheric dynamics and aurorae are domina

212 Jupiter's magnetotail is the largest cohesive structure

213 This is a weak equivalent of Jupiter's main oval, its relative dimness being due to t

214 Jupiter's main ring shows vertical corrugations reminisc

215 on several moons of the outer planets, with Jupiter's moon Europa having received the most attention

216 We report far-ultraviolet observations of Jupiter's moon Europa taken by Space Telescope Imaging S

217 Jupiter's moon Io is known to host active volcanoes.

218 On Jupiter's moon Io, volcanic plumes and evaporating lava

219 te observations of other icy bodies, such as Jupiter's moons Europa and Ganymede, and suggestive of a

220 reminiscent of the Laplace resonance linking Jupiter's moons Io, Europa and Ganymede.

221 Observations of Jupiter's nightside airglow (nightglow) and aurora obtai

222 that inner Oort Cloud objects can penetrate Jupiter's orbit via a largely unexplored dynamical pathw

223 Images of Jupiter's poles show a chaotic scene, unlike Saturn's po

224 Jupiter's relatively steady main aurora has a power dens

225 We exploited Jupiter's rotating magnetic field as a sounding signal a

226 emission residing just outside the orbit of Jupiter's satellite Europa.

227 s that the passage of ring particles through Jupiter's shadow creates the Thebe extension and fully a

228 spacecraft's encounter with Amalthea, one of Jupiter's small inner moons, on 5 November 2002 yield a

229 Near-infrared spectra of Jupiter's small inner satellites Amalthea and Thebe are

230 acecraft measurements of infrared spectra of Jupiter's stratosphere.

231 ata suffer from poor vertical resolution and Jupiter's stratospheric wind velocities have not yet bee

232 the discovery of mass anomalies on Ganymede, Jupiter's third and largest Galilean satellite.

233 esults indicate that the interaction between Jupiter's upper atmosphere and near-space environment is

234 to the lack of as large a source of ions as Jupiter's volcanic moon Io.

235 rring climate cycle which will cause most of Jupiter's vortices to disappear within the next decade.

236 plications for the stability and dynamics of Jupiter's weather layer.

237 We report findings on Jupiter's zonal winds, convective storms, low-latitude u

238 forcing, and the auroral spectrum resembles Jupiter's.

239 ratio on Saturn is seven times solar, twice Jupiter's.

240 ave acceleration could also be important for Jupiter, Saturn and other astrophysical objects with mag

241 ults presented have potential application to Jupiter, Saturn and other magnetized astrophysical objec

242 erall properties of the satellite systems of Jupiter, Saturn and Uranus arise naturally, and suggest

243 ous ultraviolet imaging we find that, unlike Jupiter, Saturn's aurorae respond strongly to solar wind

244 han being intermediate between the Earth and Jupiter, Saturn's auroral emissions behave fundamentally

245 to those observed at bow shocks upstream of Jupiter, Saturn, Uranus and Neptune.

246 masses almost equal to 5 to 20 times that of Jupiter, showing they bridge the gap between hotter brow

247 orbiting near hot Jupiter planet candidates (Jupiter-size candidates with orbital periods near 3 d) i

248 st decade, observations of giant exoplanets (Jupiter-size) have provided key insights into their atmo

249 detected atomic and molecular absorption in Jupiter-sized exoplanets, but intense efforts to measure

250 of Earth and Neptune substantially outnumber Jupiter-sized planets.

251 discovery of 23 new irregular satellites of Jupiter, so increasing the total known population to 32.

252 , similar to the CVD event rate noted in the JUPITER study placebo group (1.36% per year over 1.9 yea

253 Questions remain after the JUPITER study, including whether the observed cardiovasc

254 the L4 and L5 stable Lagrange points of the Jupiter-Sun system (leading and following Jupiter by 60

255 ubsystem acquired about 26,000 images of the Jupiter system as the spacecraft encountered the giant p

256 loss of vast numbers of heavy ions from the Jupiter system.

257 the planet that channels material out of the Jupiter system.

258 ation in this system (and possibly other hot-Jupiter systems) must be much weaker than in the Solar S

259 -orbit misalignments are not confined to hot-Jupiter systems.

260 y flux from discrete acceleration is less at Jupiter than that caused by broadband or stochastic proc

261 Our results reveal a diverse group of hot Jupiters that exhibit a continuum from clear to cloudy a

262 The 'hot Jupiters' that abound in lists of known extrasolar plane

263 of rosuvastatin were 50% of that observed in JUPITER, the incremental cost-effectiveness ratio would

264 However, in the case of the hot Jupiter, the innermost planet was Jupiter (rather than M

265 The age of Jupiter, the largest planet in our Solar System, is stil

266 sibly correlated with Europa's distance from Jupiter through tidal stress variations.

267 nt results comparing the inclinations of hot Jupiters thus produced with observations.

268 at (NNT) by applying the benefit recorded in JUPITER to the event rates within each CAC strata.

269 objects that are more than 10x as massive as Jupiter, to intermediate-mass Neptune-like objects with

270 y healthy men and women participating in the JUPITER trial (87% of full cohort), we prospectively ass

271 This secondary analysis of the JUPITER trial (a placebo-controlled randomized clinical

272 ssed in 9612 multiethnic participants in the JUPITER trial (Justification for the Use of Statins in P

273 months in a nested case-control study of the JUPITER trial (Justification for the Use of Statins in P

274 of treatment effectiveness were based on the JUPITER trial and were varied in sensitivity analyses.

275 We addressed, using the JUPITER trial cohort, whether this association remains w

276 The JUPITER trial found that rosuvastatin reduces vascular e

277 Myalgia was studied in JUPITER trial participants.

278 The JUPITER trial showed that some patients with LDL-cholest

279 dertook an analysis of participants from the JUPITER trial to address the balance of vascular benefit

280 cipants in the randomised placebo-controlled JUPITER trial were adults without diabetes or previous c

281 In the randomised, double-blind JUPITER trial, 17,603 men and women without previous car

282 For 17,802 patients in the JUPITER trial, rosuvastatin 20 mg per day reduced the in

283 to 20 mg/d of rosuvastatin or placebo in the JUPITER trial.

284 Intervention Trial Evaluating Rosuvastatin (JUPITER) trial (NCT00239681).

285 Intervention Trial Evaluating Rosuvastatin (JUPITER) trial before randomization to rosuvastatin 20 m

286 Intervention Trial Evaluating Rosuvastatin (JUPITER) trial of 17,802 initially healthy men and women

287 Intervention Trial Evaluating Rosuvastatin (JUPITER) trial of rosuvastatin users identified a sub-ge

288 Intervention Trial Evaluating Rosuvastatin (JUPITER) trial.

289 lation that is several times larger than the Jupiter Trojans.

290 identified lightning at high latitudes above Jupiter up to 80 degrees N and 74 degrees S.

291 -wavelength photometry of the transiting hot-Jupiter WASP-12b that reveals C/O >/= 1 in its atmospher

292 In a population eligible for JUPITER, we established whether coronary artery calcium

293 rocesses are solar wind driven, and those of Jupiter, where processes are driven by a large source of

294 rted into a true mass of 1.85(-0.42)(+0.52)M(Jupiter), which implies that it is a planet, not a brown

295 anomalously large radius (1.35 times that of Jupiter), which may be the result of ongoing tidal dissi

296 aturn has more prograde irregular moons than Jupiter, which we can explain as a result of the chaotic

297 n Enceladus and Saturn like that which links Jupiter with Io, Europa and Ganymede.

298 resent evidence that observed eccentric warm Jupiters with eccentric giant companions have mutual inc

299 In contrast, comparison studies of warm Jupiters (with slightly larger orbits) and hot Neptune-s

300 Absolute CVD rates (per 100 person-years) in JUPITER women for rosuvastatin and placebo (0.57 and 1.0