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4660 Nereus

Near-Earth asteroid

4660 Nereus

Near-Earth asteroid

FieldValue
minorplanetyes
name4660 Nereus
imageNereus Goldstone PIA24566 animated.gif
captionNereus imaged by NASA's Goldstone Solar System Radar on its close approach in 2021
background#FFC2E0
discovery_ref
discovererEleanor F. Helin
discovery_site1.22-m Samuel Oschin telescope
discovered28 February 1982
mpc_name(4660) Nereus
named_afterΝηρεύς Nēreús
mp_category
PHA
pronounced
orbit_ref
epoch2021-Jul-01 (JD 2459396.5)
observation_arc14647 days (40.10 yr)
uncertainty0
moid0.0031 AU
aphelion2.0250 AU
perihelion0.95287 AU
semimajor1.4889 AU
eccentricity0.36004
period1.82 yr (663.62 d)
inclination1.4316°
asc_node314.41°
mean_anomaly256.71°
arg_peri158.12°
dimensions{{Ubl
X {{}}
Y {{}}
Z {{}}
sidereal_day15.16
pole_ecliptic_lat+80°
pole_ecliptic_lon+25°
albedo
spectral_typeXe
abs_magnitude
magnitude12.6 (2021 peak)
9.8 (2060 peak)
mean_radius0.165 km
surface_area
volume
mean_motion/ day
rotation15.1 h

PHA | X
| Y
| Z
9.8 (2060 peak)

4660 Nereus (provisional designation 1982 DB) is a small (about 0.33 km) asteroid. It was discovered by Eleanor F. Helin on 28 February 1982, approximately a month after it passed 4.1 e6km from Earth.

Nereus is potentially an important asteroid with a high albedo. It is an Apollo and Mars-crosser, with an orbit that frequently comes close to Earth, and because of this it is exceptionally accessible to spacecraft. Indeed, because of its small size and close orbit, its delta-V for rendezvous of ~5 km/s is smaller than the Moon's, which is about 6.3 km/s.

Nereus makes seven approaches to Earth of less than 5 million km between 1900 and 2100. The closest will be on 14 February 2060, at 1.2 million km. The most recent closest approach was on 11 December 2021, when it was 3.9 million km away. During the 2021 approach, the asteroid peaked around apparent magnitude 12.6, requiring a telescope with around a 100mm objective lens to be visually seen. Its orbital period of 1.82 yr also puts it somewhat near a 2:1 orbital resonance with Earth, which means that an approximately 4-year mission could depart for and return from the asteroid on relatively near passes to the Earth.

Nereus is classified as a potentially hazardous asteroid (PHA), due to both its absolute magnitude (H ≤ 22) and its minimum orbit intersection distance (MOID ≤ 0.05 AU).

DateJPL SBDB
nominal geocentric
distanceuncertainty
region
(3-sigma)
2021-12-11± 3 km
2060-02-14± 234 km
2166-02-03± 261 thousand km

The asteroid is classified as E-type, so it could be potentially associated with aubrite meteorites (enstatite achondrites).

Name

Although the discoverer is given the opportunity to name the asteroid, Helin donated naming rights to the Planetary Society which organized a naming contest.

The winner, Robert M. Cutler, then an employee of NASA contractor The MITRE Corporation, named the asteroid after the ancient Greek proto-god Nereus who had characteristics later attributed to Apollo (prophecy) and Poseidon (a sea god similar to Nereus but with legs rather than a fish tail).

Physical characteristics

Collage of Nereus radar images from Goldstone in November 2021

Nereus has been imaged by radar, revealing a slightly elongated shape which would allow for stable orbits around it. More recent work on the analysis of the radar data gives a much more detailed shape for Nereus as well as a fairly detailed terrain map of the surface.

Nereus has a generally ellipsoidal shape with dimensions of . On the ends of its longest axis, one end appears narrower and rounder than the other, larger end, making it more of an egg shape. The larger end also appears to have a flatter region on one side of it. Nereus rotates about an axis roughly perpendicular to its longest axis much like a silver spoon spinning on a table.

Exploration

Nereus was proposed for visitation by both the private Near Earth Asteroid Prospector (NEAP) probe, and the Japanese sample return mission Hayabusa. However, the NEAP probe was not realized, and the Hayabusa's launch was delayed by 10 months and the probe had to be redirected to 25143 Itokawa.

4660 Nereus was considered as a flyby target of the NEAR robotic spacecraft mission. NEAR was eventually launched, but visited 253 Mathilde and 433 Eros.

References

References

  1. {{MW. Nereus
  2. "NEO Groups". [[NASA]].
  3. Helin, Eleanor F. (Jan/Feb 1991), "Eureka! The Recovery of 1982DB," pp. 12–16, Planetary Report, Planetary Society, Pasadena, CA.
  4. Delbo, Marco. (November 2003). "Keck observations of near-Earth asteroids in the thermal infrared". [[Icarus (journal).
  5. [http://adsabs.harvard.edu/abs/1993STIA...9581370F Extended-mission opportunities for a Discovery-class asteroid rendezvous mission]
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