 S/2002 N 5 imaged by theVery Large Telescope in September 2002 | |
| Discovery[1][2] | |
|---|---|
| Discovered by | Matthew Holman John J. Kavelaars Tommy Grav Wesley Fraser |
| Discovery site | Cerro Tololo Obs. |
| Discovery date | 14 August 2002 |
| Designations | |
| c02N4[3] | |
| Orbital characteristics[4] | |
| Epoch 1 January 2020 (JD 2458849.5) | |
| Observation arc | 21.22yr (7,752d) |
| Satellite of | Neptune |
| Group | Sao group |
| Proper orbital elements | |
Propersemi-major axis | 23,414,700 km (0.156518 AU) AU |
Propereccentricity | 0.433 |
Properinclination | 46.3° (toecliptic) |
Propermean motion | 41.6561611 deg / yr |
Properorbital period | 8.64218yr (3156.556d) |
Precession ofperihelion | 451.707549 arcsec / yr |
Precession of theascending node | 415.317659 arcsec / yr |
| Physical characteristics | |
| 24–38 km[a] 23 km[5][6] | |
| 25.9 (average)[5] | |
| 11.2[1] | |
S/2002 N 5 is a progradeirregular satellite ofNeptune. It was discovered on 14 August 2002 byMatthew Holman,John J. Kavelaars, Tommy Grav, and Wesley Fraser using the 4.0-meterVíctor M. Blanco Telescope atCerro Tololo Observatory,Chile, but it becamelost and was not observed again untilScott S. Sheppard rediscovered it on 3 September 2021. The discovery of S/2002 N 5 was announced on 23 February 2024, after observations were collected over a long enough time to confirm the satellite's orbit.[1] S/2002 N 5 orbits Neptune at an average distance of over 23 million km (14 million mi) and takes almost 9 Earth years to complete its orbit.
S/2002 N 5 was first observed on 14 August 2002 by Matthew Holman and collaborators, during their search for Neptunian irregular moons using the 4.0-mVíctor M. Blanco Telescope atCerro Tololo Observatory,Chile.[3]: 866 Holman's team was able to detect this faint moon through theshift-and-add technique, in which they took many long-exposure telescope images, aligned and shifted them to follow Neptune's motion, and then added them together to create a single deep image that would show Neptunian moons as points of light against trailed background stars and galaxies.[3]: 865 The moon was given the temporary designation "c02N4" and was among the faintest of the five Neptunian moons that Holman's team discovered in their search, which includedHalimede,Sao,Laomedeia, andNeso.[3]: 866 While four of these moons were successfully reobserved and subsequently announced, S/2002 N 5 was only reobserved once on 3 September 2002 by the 8.2-mVery Large Telescope atEuropean Southern Observatory.[1][3]: 866 Further attempts to reobserve S/2002 N 5 were unsuccessful.[3]: 866 With very few observations, S/2002 N 5's orbit could not be confirmed and it became alost moon.[3]: 866 [6]
S/2002 N 5 remained unobserved for 19 years since its last observation by Holman's team in September 2002.[1] On 3 September 2021,Scott S. Sheppard rediscovered S/2002 N 5 while searching for Neptunian irregular moons with the 6.5-mMagellan–Baade Telescope atLas Campanas Observatory, Chile.[1][6] Like Holman's team, Sheppard used the shift-and-add technique to detect S/2002 N 5.[6] From September 2021 to November 2023, Sheppard and his collaboratorsDavid J. Tholen,Chad Trujillo, and Patryk S. Lykawka conducted follow-up observations of S/2002 N 5 using the Magellan–Baade Telescope and the 8.2-mSubaru Telescope atMauna Kea, Hawaii to determine the moon's orbit and ensure it would not be lost.[1][6] After Sheppard's follow-up observations concluded, his team was able to link the moon back to its original discovery observations from 2002.[6] S/2002 N 5 andS/2021 N 1, another Neptunian irregular moon discovered by Sheppard's team, were both confirmed and announced by theMinor Planet Center on 23 February 2024, bringing Neptune's number of known moons from 14 to 16.[1]
S/2002 N 5 is anirregular moon of Neptune, since it has a distant, highlyelliptical, and highlyinclined orbit. Irregular moons are loosely bound by Neptune's gravity because of their great distance from the planet, so their orbits are frequentlyperturbed by the gravity of the Sun and other planets.[7]: 2 This results in significant changes in the orbits of irregular moons over short periods of time, so a simpleKeplerian elliptical orbit cannot accurately describe the long-term orbital motions of irregular moons. Instead,proper or average orbital elements are used to describe the long-term orbits of irregular moons more accurately, since these are calculated by averaging out the perturbed orbit over a long period of time.[7]: 4
Over an 800-year time span from 1600 to 2400, S/2002 N 5's averagesemi-major axis or orbital distance from Neptune is 23.4 million km (14.5 million mi; 0.156 AU), with an averageorbital period of 8.6Earth years.[4] S/2002 N 5 has an averageorbital eccentricity of 0.43 and an averageinclination of 46.3° with respect to theecliptic, or the plane of Earth's orbit.[4] Since S/2002 N 5's orbital inclination is less than 90°, the moon has aprograde orbit, meaning it orbits in the same direction as Neptune's orbit around the Sun.[5] Due to perturbations, S/2002 N 5's orbital elements fluctuate over time: its semi-major axis can range from 23.3 to 23.6 million km (14.5 to 14.7 million mi), eccentricity from 0.24 to 0.67, and inclination from 37° to 50°.[8] S/2002 N 5's orbit exhibitsnodal precession with an average period of about 3,100 Earth years andapsidal precession with an average period of about 2,900 Earth years.[4]
S/2002 N 5 is part of the Sao group, a cluster of distant prograde irregular moons of Neptune that includesLaomedeia and the group's namesakeSao.[5] The moons of the Sao group have orbital elements that are clustered with semi-major axes between 22–24 million km (14–15 million mi), eccentricities between 0.3 and 0.5, and inclinations between 30° and 50°.[5] Like all other irregular moon groups, the Sao group is thought to have formed from the destruction of a larger captured moon of Neptune due to asteroid and cometimpacts, which left many fragments in similar orbits around Neptune.[6]
S/2002 N 5 is very faint with an averageapparent magnitude of 25.9, so it could only be observed with long-exposure imaging by large-aperture telescopes like the Subaru Telescope.[5][6] Nothing is known about S/2002 N 5's physical properties other than itsabsolute magnitude of 11.2, which can be used to estimate the moon's diameter.[1] Assuming ageometric albedo range of 0.04–0.10 that is typical for most irregular moons,[9] S/2002 N 5 has a diameter between 24–38 km (15–24 mi).[a] Sheppard estimates the diameter to be 23 km, which if correct would make S/2002 N 5 one of the smallest known satellites orbiting Neptune.[5][6]
Listed in approximately increasing distance fromNeptune | |||||||||||
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