Neso (moon)

Neso
	Neso imaged by the Very Large Telescope's FORS1 imager in September 2002
Discovery
Discovered by	M. Holman et al.; B. Gladman et al.;
Discovery site	Cerro Tololo Obs.
Discovery date	14 August 2002
Designations
Designation	Neptune XIII
Pronunciation	/ˈniːsoʊ/
Named after	Νησώ Nēsō
Alternative names	S/2002 N 4
Adjectives	Nesoan /nɪˈsoʊ.ən/ or Nesoian /nɪˈsoʊ.iən/
Orbital characteristics
	Epoch 1 January 2000 (Proper orbital element)
Observation arc	19.96 yr (7,292 days)
Mean anomaly	11.2° (proper)
Satellite of	Neptune
Group	Neso group
Proper orbital elements
Proper semi-major axis	49,598,300 km = 0.332 AU
Proper eccentricity	0.455
Proper inclination	126.9°
Proper mean motion	13.4246 deg / yr
Proper orbital period	26.81644 yr; (9794.705 d)
Precession of the ascending node	1161.3684 arcsec / yr
Physical characteristics
Mean diameter	60 km (for albedo 0.04)
Albedo	0.04 (assumed)
Spectral type	V–R = 0.58±0.13; V–I = 1.0±0.4; R–I = 0.7±0.4
Apparent magnitude	25.6±0.3 (V-band)
Absolute magnitude (H)	10.67

Neso /ˈniːsoʊ/, also known as Neptune XIII, is the second-outermost known natural satellite of Neptune, after S/2021 N 1. It is a retrograde irregular moon discovered by Matthew J. Holman, Brett J. Gladman, et al. on 14 August 2002, though it went unnoticed until 2003.^[2]^[8] Neso is the second-most distant moon of Neptune, with an average orbital distance of over 49 million km. At its farthest point of its orbit, the satellite is more than 72 million km from Neptune. This distance exceeds Mercury's aphelion, which is approximately 70 million km from the Sun.

Neso is also the moon with the second-longest orbital period, 26.67 years. It follows a retrograde, highly inclined, and highly eccentric orbit illustrated on the diagram in relation to other irregular satellites of Neptune. The satellites above the horizontal axis are prograde, the satellites beneath it are retrograde. The yellow segments extend from the pericentre to the apocentre, showing the eccentricity.

Neso is affected by the Kozai mechanism.^[9]

Neso is about 60 km (37 mi) in diameter based on an assumed albedo of 0.04.

Given the similarity of the orbit's parameters with Psamathe (S/2003 N 1), it was suggested that both irregular satellites could have a common origin in the break-up of a larger moon.^[5]

Neso is named after one of the Nereids. Before it was officially named on 3 February 2007 (IAUC 8802), Neso was known by its provisional designation, S/2002 N 4.

References

^ JPL (21 July 2011). "Planetary Satellite Discovery Circumstances". Jet Propulsion Laboratory. Retrieved 24 October 2011.
^ a b Green, Daniel W. E. (1 October 2003). "S/2001 U 2 and S/2002 N 4". IAU Circular. 8213. Retrieved 24 October 2011.
^ a b "Natural Satellites Ephemeris Service". Minor Planet Center. Retrieved 14 June 2023. Selection of Objects → "All Neptunian outer irregular satellites" → Check "I require Orbital Elements" → Get Information
^ Jacobson, R. A. (2008). "NEP078 – JPL satellite ephemeris". Planetary Satellite Mean Orbital Parameters. Retrieved 23 September 2009.
^ a b c Sheppard, Scott S.; Jewitt, David C.; Kleyna, Jan (2006). "A Survey for "Normal" Irregular Satellites around Neptune: Limits to Completeness". The Astronomical Journal. 132 (1): 171–176. arXiv:astro-ph/0604552. Bibcode:2006AJ....132..171S. doi:10.1086/504799. S2CID 154011.
^ Graykowski, Ariel; Jewitt, David (April 2018). "Colors and Shapes of the Irregular Planetary Satellites". The Astronomical Journal. 155 (4): 10. arXiv:1803.01907. Bibcode:2018AJ....155..184G. doi:10.3847/1538-3881/aab49b. 184.
^ a b c Maris, Michele; Carraro, Giovanni; Melita, Mario; Parisi, Gabriela (March 2018). "Multicolor Photometry of the Neptune Irregular Satellite Neso". Research Notes of the American Astronomical Society. 2 (1). arXiv:1803.07957. Bibcode:2018RNAAS...2...42M. doi:10.3847/2515-5172/aab7fc. 42.
^ Holman, M. J.; Kavelaars, J. J.; Grav, T.; et al. (2004). "Discovery of five irregular moons of Neptune" (PDF). Nature. 430 (7002): 865–867. Bibcode:2004Natur.430..865H. doi:10.1038/nature02832. PMID 15318214. S2CID 4412380. Retrieved 24 October 2011.
^ Brozović, Marina; Jacobson, Robert A.; Sheppard, Scott S. (10 March 2011). "THE ORBITS OF NEPTUNE'S OUTER SATELLITES". The Astronomical Journal. 141 (4): 135. doi:10.1088/0004-6256/141/4/135. ISSN 0004-6256.

MPC: Natural Satellites Ephemeris Service
Mean orbital parameters from JPL

External links

Matthew Holman's Neptune's page
David Jewitt's pages
Scott Sheppard's pages
Neso in Fiction

[JPL-Discoverers-1] JPL (21 July 2011). "Planetary Satellite Discovery Circumstances". Jet Propulsion Laboratory. Retrieved 24 October 2011.

[IAUC_8213-2] Green, Daniel W. E. (1 October 2003). "S/2001 U 2 and S/2002 N 4". IAU Circular. 8213. Retrieved 24 October 2011.

[MPC-NatSats-3] "Natural Satellites Ephemeris Service". Minor Planet Center. Retrieved 14 June 2023. Selection of Objects → "All Neptunian outer irregular satellites" → Check "I require Orbital Elements" → Get Information

[JPL-Jacobson2008-4] Jacobson, R. A. (2008). "NEP078 – JPL satellite ephemeris". Planetary Satellite Mean Orbital Parameters. Retrieved 23 September 2009.

[SheppardJewittKleyna2006-5] Sheppard, Scott S.; Jewitt, David C.; Kleyna, Jan (2006). "A Survey for "Normal" Irregular Satellites around Neptune: Limits to Completeness". The Astronomical Journal. 132 (1): 171–176. arXiv:astro-ph/0604552. Bibcode:2006AJ....132..171S. doi:10.1086/504799. S2CID 154011.

[Graykowski2018-6] Graykowski, Ariel; Jewitt, David (April 2018). "Colors and Shapes of the Irregular Planetary Satellites". The Astronomical Journal. 155 (4): 10. arXiv:1803.01907. Bibcode:2018AJ....155..184G. doi:10.3847/1538-3881/aab49b. 184.

[Maris2018-7] Maris, Michele; Carraro, Giovanni; Melita, Mario; Parisi, Gabriela (March 2018). "Multicolor Photometry of the Neptune Irregular Satellite Neso". Research Notes of the American Astronomical Society. 2 (1). arXiv:1803.07957. Bibcode:2018RNAAS...2...42M. doi:10.3847/2515-5172/aab7fc. 42.

[HolmanKavelaarsGrav2004-8] Holman, M. J.; Kavelaars, J. J.; Grav, T.; et al. (2004). "Discovery of five irregular moons of Neptune" (PDF). Nature. 430 (7002): 865–867. Bibcode:2004Natur.430..865H. doi:10.1038/nature02832. PMID 15318214. S2CID 4412380. Retrieved 24 October 2011.

[9] Brozović, Marina; Jacobson, Robert A.; Sheppard, Scott S. (10 March 2011). "THE ORBITS OF NEPTUNE'S OUTER SATELLITES". The Astronomical Journal. 141 (4): 135. doi:10.1088/0004-6256/141/4/135. ISSN 0004-6256.

Discovery^[1]^[2]
Neso imaged by the Very Large Telescope's FORS1 imager in September 2002
Discovered by	M. Holman et al. B. Gladman et al.
Discovery site	Cerro Tololo Obs.
Discovery date	14 August 2002
Designations
Designation	Neptune XIII
Pronunciation	/ˈniːsoʊ/
Named after	Νησώ Nēsō
Alternative names	S/2002 N 4
Adjectives	Nesoan /nɪˈsoʊ.ən/ or Nesoian /nɪˈsoʊ.iən/
Orbital characteristics
Epoch 1 January 2000 (Proper orbital element)
Observation arc	19.96 yr (7,292 days)^[3]
Mean anomaly	11.2° (proper)
Satellite of	Neptune
Group	Neso group
Proper orbital elements^[4]
Proper semi-major axis	49,598,300 km = 0.332 AU
Proper eccentricity	0.455
Proper inclination	126.9°
Proper mean motion	13.4246 deg / yr
Proper orbital period	26.81644 yr (9794.705 d)
Precession of the ascending node	1161.3684 arcsec / yr
Physical characteristics
Mean diameter	60 km (for albedo 0.04)^[5]
Albedo	0.04 (assumed)^[5]
Spectral type	V–R = 0.58±0.13^[6] V–I = 1.0±0.4^[7] R–I = 0.7±0.4^[7]
Apparent magnitude	25.6±0.3 (V-band)^[7]
Absolute magnitude (H)	10.67^[3]

Neso (moon)

See also

References

External links