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2035 Stearns

Mars-crossing asteroid


Mars-crossing asteroid

FieldValue
minorplanetyes
name2035 Stearns
background#FA8072
discovery_ref
discovererJ. B. Gibson
discovery_siteEl Leoncito Complex
discovered21 September 1973
mpc_name(2035) Stearns
alt_names1973 SC1973 UG
named_afterCarl Leo Stearns
(American astronomer)
mp_categoryMars-crosser
Hungaria
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc44.35 yr (16,199 d)
aphelion2.1317 AU
perihelion1.6366 AU
semimajor1.8841 AU
eccentricity0.1314
period2.59 yr (945 d)
mean_anomaly134.07°
mean_motion/ day
inclination27.751°
asc_node77.035°
arg_peri200.71°
moid0.6305 AU (245 LD)
mars_moid0.1655 AU
mean_diameter
(derived)
rotation
albedo(assumed)
spectral_typeTholen E
SMASS Xe
B–V 0.737
U–B 0.280
V–R
abs_magnitude12.61
13.0

(American astronomer) Hungaria (derived)

SMASS Xe B–V 0.737 U–B 0.280 V–R
13.0

2035 Stearns, provisional designation , is a bright Hungaria asteroid and sizable Mars-crosser inside the inner regions of the asteroid belt, approximately 6 km in diameter. It was discovered on 21 September 1973, by American astronomer James Gibson at the Leoncito Astronomical Complex in Argentina. The transitional E-type asteroid has a long rotation period of 93 hours. It was named after American astronomer Carl Leo Stearns.

Orbit and classification

Stearns is a dynamical Hungaria asteroid, a large group that forms the innermost dense concentration of asteroids in the Solar System. It is also a Mars-crossing asteroid, a member of the dynamically unstable group, located between the main belt and near-Earth populations, and crossing the orbit of Mars at 1.666 AU.

The asteroid orbits the Sun in the inner main-belt at a distance of 1.64–2.13 AU once every 2 years and 7 months (945 days; semi-major axis of 1.88 AU). Its orbit has an eccentricity of 0.13 and an inclination of 28° with respect to the ecliptic.

The body's observation arc begins with a precovery taken at Palomar Observatory in January 1954, nearly 20 years prior to its official discovery observation at Leoncito.

Physical characteristics

In the Tholen classification, Stearns is a bright E-type asteroid. while in the SMASS classification and Bus-DeMeo taxonomy, it is an Xe-subtype that transitions from the X-type to the E-type.

Rotation period

Several rotational lightcurve of Stearns have been obtained from photometric observations since 1988. Analysis of the best-rated lightcurve by Robert Stephens at the Center for Solar System Studies gave a rotation period of 93 hours with a brightness amplitude of 0.20 magnitude (). This makes the asteroid as close slow rotator.

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Stearns measures between 4.82 and 6.00 kilometers in diameter and its surface has an albedo between 0.443 and 0.65. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for members of the Hungaria family of 0.40, and derives a diameter of 5.28 kilometers based on an absolute magnitude of 13.0.

Naming

This minor planet was named after Carl Leo Stearns (1892–1972), American astronomer at Wesleyan University and Van Vleck Observatory who measured a large number of stellar parallaxes. The official was published by the Minor Planet Center on 1 November 1978 (M.P.C. 4548). The lunar crater Stearns was also named in his honor.

Notes

References

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