Skip to content
Surf Wiki
Save to docs
general/background-asteroids

From Surf Wiki (app.surf) — the open knowledge base

789 Lena

Main-Belt Asteroid


Summary

Main-Belt Asteroid

FieldValue
minorplanetyes
name789 Lena
background#D6D6D6
discovery_ref
discovered24 June 1914
discovererG. Neujmin
discovery_siteSimeiz Obs.
mpc_name(789) Lena
alt_names1914 UU1970 CE
pronounced
named_afterElena Neujmina
(discoverer's family)
mp_categorymain-belt(middle)
orbit_ref
epoch16 February 2017 (JD 2457800.5)
uncertainty0
observation_arc81.69 yr (29,837 days)
aphelion3.0817 AU
perihelion2.2907 AU
semimajor2.6862 AU
eccentricity0.1472
period4.40 yr (1,608 days)
mean_anomaly110.02°
mean_motion/ day
inclination10.781°
asc_node232.62°
arg_peri44.006°
dimensionskm
km
24.18 km (calculated)
rotationh
h
h
h
albedo0.10 (assumed)
spectral_typeSMASS = XMX
abs_magnitude10.911.2

(discoverer's family)

km 24.18 km (calculated) h h h

789 Lena, provisional designation **, is a metallic asteroid from the middle region of the asteroid belt, approximately 24 kilometers in diameter. It was discovered on 24 June 1914, by Soviet–Russian astronomer Grigory Neujmin at Simeiz Observatory on the Crimean peninsula, and named after the discoverer's mother.

Orbit and classification

Lena orbits the Sun in the middle main-belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,608 days). Its orbit has an eccentricity of 0.15 and an inclination of 11° with respect to the ecliptic. Lenas observation arc begins with its first used observation made at Yerkes Observatory in 1935, or 21 years after its official discovery observation at Simeiz.

Although its orbital elements resemble those of the asteroids in the Eunomia family, true members of this family have a S-type composition, so it is almost certainly an unrelated interloper.

Physical characteristics

In the SMASS taxonomy, Lena is an X-type asteroid. It has also been characterized as a metallic M-type asteroid by NASA's Wide-field Infrared Survey Explorer (WISE).

Rotation period

In 1993, a rotational lightcurve which was later proven incorrect, was obtained from photometric observations at the Félix Aguilar Observatory, Argentina. It gave an unusual lightcurve, indicating a very irregular shape and/or a relatively long rotation period of 22 hours with an exceptionally high amplitude of 1.5 in magnitude ().

In August and September 2007, two reliable lightcurves were obtained by Italian astronomer Silvano Casulli and by members at the U.S.Oakley Observatory. Lightcurve analysis gave a period of and hours, with a brightness variation of 0.50 and of 0.40 magnitude, respectively ().

Diameter and albedo

According to the space-based surveys carried out by the Japanese Akari satellite and the NEOWISE mission of the WISE telescope, Lena measures between 20.6 and 23.9 kilometers in diameter, and its surface has an albedo of 0.137–0.186. The Collaborative Asteroid Lightcurve Link assumes a much lower albedo of 0.10 and calculates a diameter of 24.2 kilometer, as the lower the albedo (reflectivity), the larger a body's diameter, at a constant absolute magnitude (brightness).

Naming

This minor planet was named in honor of Elena ("Lena") Petrovna Neujmina (1860–1942), mother of the discovering astronomer Grigory Neujmin.

Notes

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
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.

Want to explore this topic further?

Ask Mako anything about 789 Lena — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.

Report