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1121 Natascha

Main-belt asteroid


Summary

Main-belt asteroid

FieldValue
minorplanetyes
name1121 Natascha
background#D6D6D6
image001121-asteroid shape model (1121) Natascha.png
captionShape model of Natascha from its lightcurve
discovery_ref
discovererP. Shajn
discovery_siteSimeiz Obs.
discovered11 September 1928
mpc_name(1121) Natascha
alt_names1928 RZA918 EK
named_afterNatasha Tichomirova
(daughter of G. Neujmin)
mp_categorymain-belt(inner)
backgroundAstraea
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc87.68 yr (32,024 days)
aphelion2.9500 AU
perihelion2.1428 AU
semimajor2.5464 AU
eccentricity0.1585
period4.06 yr (1,484 days)
mean_anomaly285.31°
mean_motion/ day
inclination6.1646°
asc_node357.91°
arg_peri50.379°
mean_diameterkm
km
14.89 km (calculated)
rotation
pole_ecliptic_lat{{plainlist
* (16.0°, 59.0°) (λ<sub>1</sub>/β<sub>1</sub>)<ref name"Ferret" /
* (209.0°, 50.0°) (λ<sub>2</sub>/β<sub>2</sub>)<ref name"Ferret" /}}
albedo
0.20 (assumed)
spectral_typeS (assumed)
abs_magnitude11.4011.511.80

(daughter of G. Neujmin) backgroundAstraea km 14.89 km (calculated)

  • (16.0°, 59.0°) (λ1/β1)
  • (209.0°, 50.0°) (λ2/β2)}} 0.20 (assumed)

1121 Natascha (prov. designation: ) is a background asteroid from the central regions of the asteroid belt. It was discovered on 11 September 1928, by Soviet astronomer Pelageya Shajn at the Simeiz Observatory on the Crimean peninsula. The presumed S-type asteroid has rotation period of 13.2 hours and measures approximately 14 km in diameter. It was named for Natasha Tichomirova, daughter of astronomer Grigory Neujmin.

Orbit and classification

Natascha is a non-family asteroid from the main belt's background population. Conversely, the asteroid is also considered a core member of the disputed Astraea family. It orbits the Sun in the central main-belt at a distance of 2.1–3.0 AU once every 4 years and 1 month (1,484 days; semi-major axis of 2.55 AU). Its orbit has an eccentricity of 0.16 and an inclination of 6° with respect to the ecliptic. The asteroid was first observed as at Simeiz Observatory in March 1918. The body's observation arc begins at Heidelberg Observatory in February 1930, or 17 months after its official discovery observation at Simeiz.

Naming

This minor planet was named as a birthday present for Soviet hydrogeologist Natasha (Natalia) Tichomirova, daughter of Grigory Neujmin, who was an astronomer at the discovering Simeiz Observatory and prolific discoverer of minor planets himself (AN 240;409). The author of the Dictionary of Minor Planet Names, Lutz Schmadel, learned about the naming circumstances from Crimean astronomers N. Solovaya, Nataliya Sergeevna Samoilova-Yakhontova and Nikolai Chernykh (also see and ).

Physical characteristics

Natascha is an assumed, stony S-type asteroid.

Rotation period and poles

In May 2012, a rotational lightcurve of Natascha was obtained from photometric observations by astronomers at the Oakley Southern Sky Observatory in Australia. Lightcurve analysis gave a well-defined rotation period of 13.197 hours with a brightness variation of 0.51 magnitude (). A high brightness amplitude typically indicates a non-spherical shape.

In 2016, a modeled lightcurve was published using photometric data from the Lowell Photometric Database. Lightcurve inversion gave a concurring period of hours, as well as two spin axes of (16.0°, 59.0°) and (209.0°, 50.0°) in ecliptic coordinates (λ, β).

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Natascha measures between 12.859 and 14.52 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 14.89 kilometers based on an absolute magnitude of 11.5.

References

Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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