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....com/carnegiescience.edu/sheppard/moons/jupitermoons S.S. Sheppard (2019), Moons of Jupiter, ''Carnegie Science'', on line]</ref> ...{{IPAc-en|ˈ|n|iː|m|iː}}, also known as '''{{nowrap|Jupiter XL}}''', is a [[Prograde and retrograde motion|retrograde]] [[irregular satellite]] of [[Jupiter]]. ...

'''Sao''' {{IPAc-en|ˈ|s|eɪ|.|oʊ}} is a [[Prograde and retrograde motion|prograde]] [[irregular satellite]] of [[Neptune]]. It was discovered by [[Matthew J. Sao orbits Neptune at a distance of about 22.4 million km and is about 44 kilometers in diameter (a ...

....com/carnegiescience.edu/sheppard/moons/jupitermoons S.S. Sheppard (2019), Moons of Jupiter, ''Carnegie Science'', on line]</ref> ...|retrograde]] [[irregular satellite]] of [[Jupiter]]. It was discovered by a team of astronomers from the [[University of Hawaii]] led by [[Scott S. She ...

...Prograde and retrograde motion|prograde]] [[irregular satellite]] of the [[moons of Uranus]]. It was discovered by [[Scott S. Sheppard]], et al. in 2003 an ...t,” which was my Mom’s name, on the Web, and “Shakespeare.” And it came up with ''Much Ado about Nothing''. And I said that’s it, that’s what I’ll name it. ...

| pronounced = {{IPAc-en|θ|aɪ|ˈ|oʊ|n|iː}}<ref>Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref> ....com/carnegiescience.edu/sheppard/moons/jupitermoons S.S. Sheppard (2019), Moons of Jupiter, ''Carnegie Science'', on line]</ref> ...

...upiter]] that follow similar [[orbit]]s to Himalia and are thought to have a common origin.<ref name="SJ2003">[[Scott S. Sheppard]], [[David C. Jewitt]] ...d'''a''', Himali'''a''' and so on) for the moons in this group to indicate prograde motions of these bodies relative to Jupiter, their gravitationally central ...

...}}, also known as '''Neptune XII''', is a [[Prograde and retrograde motion|prograde]] [[irregular satellite]] of [[Neptune]]. It was discovered by [[Matthew J. It orbits Neptune at a distance of about 23,571,000&nbsp;km and is about 42 kilometers in diameter ...

| pronounced = {{IPAc-en|h|æ|l|ə|ˈ|m|iː|d|iː}}<ref>Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref> | period = 1879.08 d <br /> (5.14 [[Julian year (astronomy)|a]]) ...

| perihelion_rate = N/A ...n March 2005 after [[Horae#Descriptions|Carpo]], one of the [[Horae]], and a daughter of [[Zeus]] (Jupiter).<ref name="Gazetteer"/> ...

...pectively. The satellites with inclinations below 90° are [[prograde orbit|prograde]], those above 90° are [[retrograde motion|retrograde]]. The X-axis is labe ...eccentricities]] between 0.11 and 0.39. They take an average of 2 years to orbit Saturn. ...

{{short description|Angle between a reference plane and the plane of an orbit}} ...Fig. 1: Orbital inclination represented by '''''i''''' (dark green), along with other fundamental [[orbital parameters]]]] ...

...oʊ}}<ref>Cf. 'Themista' in {{cite book|author=Noah Webster|year=1884|title=A Practical Dictionary of the English Language}}</ref> ...|ə|n}}<ref>'Themis[t]oan' in {{cite book|author=James Hall|year=2015|title=Moons of the Solar System|page=82}}</ref> {{nowrap|Themistoian {{IPAc-en|θ|ɛ|m|ə| ...

...the [[Hubble Space Telescope]].<ref name="IAUC 8209" /> It was named after a character in [[William Shakespeare]]'s play ''[[Timon of Athens]]''.<ref na ...e interactions that cause the smaller Cupid to drift into a more dangerous orbit over this timescale.<ref name="French Showalter 2012">{{cite journal |last1 ...

...Y and X-axis, respectively. The satellites with inclinations below 90° are prograde, those above 90° are [[retrograde motion|retrograde]]. The X-axis is labele ...reserves names taken from [[Celtic mythology|Gallic mythology]] for these moons. ...

{{short description|Apparent backward motion of a planet}} ...lestial bodies relative to a gravitationally central object|Retrograde and prograde motion}} ...

...n|retrograde]] [[irregular satellite]] of [[Uranus]]. It was discovered by a group of astronomers led by Holman, ''et al.'' on 13 August 2001, and given ...pest (play)|The Tempest]]''. Trinculo is the third smallest of Uranus's 28 moons after [[Ferdinand (moon)|Ferdinand]] and [[S/2023 U 1]] and is approximatel ...

...075-ch020 |editor2=Clark, R.N. |editor3=Howett, C.J.A. |editor4=Verbiscer, A.J. |editor5=Waite, J.H. |chapter-url=https://tilmanndenk.de/wp-content/uplo ...ugust 2003, is after [[Tarvos Trigaranus|Tarvos]], a [[deity]] depicted as a [[bull]] god carrying three [[crane (bird)|cranes]] alongside its back from ...

| period = prograde, ca. 20 h ...d moon]] {{cvt|1200|by|1400|by|1600|m}}, in size) that orbits [[243 Ida]], a [[main-belt asteroid]]. It was imaged by the ''[[Galileo spacecraft|Galileo ...

| pronounced = {{IPAc-en|ˈ|d|aɪ|.|ə}}<ref>Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref> ...t S. Sheppard]], [[David C. Jewitt]], [[Yanga R. Fernández]], and [[Eugene A. Magnier]]<!-- G. for "Gene" --> ...

...Ac-en|p|r|æ|k|ˈ|s|ɪ|d|ə|k|iː}}<ref>as 'Praxidice' in Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref> ....com/carnegiescience.edu/sheppard/moons/jupitermoons S.S. Sheppard (2019), Moons of Jupiter, ''Carnegie Science'', on line]</ref> ...