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

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

2031 BAM

Asteroid


Asteroid

FieldValue
minorplanetyes
name2031 BAM
background#D6D6D6
imageOrbit of 2031 BAM.gif
captionOrbital diagram of *BAM*
discovery_ref
discovererL. Chernykh
discovery_siteCrimean Astrophysical Obs.
discovered8 October 1969
mpc_name(2031) BAM
alt_names1939 VB
1959 TW1972 NQ
named_afterBaikal–Amur Mainline
(Siberian railway line)
mp_categorymain-belt(inner)
Flora
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc77.39 yr (28,268 days)
aphelion2.6203 AU
perihelion1.8477 AU
semimajor2.2340 AU
eccentricity0.1729
period3.34 yr (1,220 days)
mean_anomaly124.02°
mean_motion/ day
inclination4.7524°
asc_node169.28°
arg_peri213.58°
dimensions7.14 km (calculated)
km
rotationh
albedo
0.24 (assumed)
spectral_typeS
abs_magnitude12.913.00

1959 TW1972 NQ (Siberian railway line) Flora km 0.24 (assumed)

2031 BAM, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 8 October 1969, by Soviet astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named for those who built the Baikal–Amur Mainline (BAM; БАМ), a Siberian railway line.

Orbit and classification

BAM is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids in the main belt. It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,220 days; semi-major axis of 2.23 AU). Its orbit has an eccentricity of 0.17 and an inclination of 5° with respect to the ecliptic.

The body's observation arc begins with its identification as at Uccle Observatory in November 1939, almost 30 years prior to its official discovery observation at Nauchnyj.

Physical characteristics

BAM has been characterized as a stony S-type asteroid by Pan-STARRS photometric survey.

Rotation period

In October 2016, a rotational lightcurve of BAM was obtained from photometric observations by amateur astronomer Matthieu Conjat. Lightcurve analysis gave a well-defined rotation period of 10.774 hours with a brightness amplitude of 0.15 magnitude ().

Diameter and albedo

According to the survey carried out by the Japanese Akari satellite, BAM measures 8.14 kilometers in diameter and its surface has an albedo of 0.170. The Collaborative Asteroid Lightcurve Link assumes a standard albedo of 0.24 – derived from 8 Flora, the parent body of the Flora family – and calculates a diameter of 7.14 kilometers based on an absolute magnitude of 12.9.

Naming

This minor planet was named after those who constructed the Baikal–Amur Mainline (BAM; БАМ) through eastern Russia from 1974 to 1986. The rail line opened in 1989, and runs between Ust-Kut (near Lake Baikal and Komsomolsk-on-Amur. The official was published by the Minor Planet Center on 1 September 1978 (M.P.C. 4482).

References

Info: 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 2031 BAM — 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