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

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

3309 Brorfelde

Hungaria asteroid from the inner regions of the asteroid belt


Hungaria asteroid from the inner regions of the asteroid belt

FieldValue
minorplanetyes
name3309 Brorfelde
background#D6D6D6
discovery_ref
discovered28 January 1982
discovererK. Jensen
K. Augustesen
discovery_siteBrorfelde Obs.
mpc_name(3309) Brorfelde
alt_names1982 BH
named_afterBrorfelde Observatory
(discovering observatory)
mp_categorymain-beltHungaria
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc35.25 yr (12,876 days)
aphelion1.9143 AU
perihelion1.7208 AU
semimajor1.8175 AU
eccentricity0.0532
period2.45 yr (895 days)
mean_anomaly76.394°
mean_motion/ day
inclination21.136°
asc_node29.797°
arg_peri218.43°
satellites1
dimensionskm
3.91 km (derived)
km
rotationh
h
h
h
h
h
h
albedo
0.2747 (derived)
spectral_typeSMASS = SS
abs_magnitude(R) (R)13.6013.713.9

K. Augustesen (discovering observatory) 3.91 km (derived) km h h h h h h 0.2747 (derived)

3309 Brorfelde, provisional designation , is a nearly spheroidal, binary Hungaria asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 28 January 1982, by Danish astronomers Kaare Jensen and Karl Augustesen at the Brorfelde Observatory near Holbæk, Denmark. It was named for the discovering observatory and the village where it is located.

Orbit and classification

Brorfelde is a bright stony asteroid and member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun at a distance of 1.7–1.9 AU once every 2 years and 5 months (895 days). Its orbit has an eccentricity of 0.05 and an inclination of 21° with respect to the ecliptic. The body's observation arc begins with its official discovery observation, as no precoveries were taken, and no prior identifications were made.

Physical characteristics

On the SMASS taxonomic scheme, Brorfelde is a common stony S-type asteroid.

Photometry

Between 2005 and 2010, astronomers Brian Warner and Petr Pravec obtained a large number of rotational lightcurves of Brorfelde. Best rated lightcurve analysis gave a rotation period between 2.5041 and 2.5046 hours with a brightness amplitude between 0.09 and 0.13 in magnitude, indicating that the body has a nearly spheroidal shape ().

These results superseded photometric observations taken by Wiesław Z. Wiśniewski in the 1990s (), and by Federico Manzini and René Roy in 2005 and 2009, respectively (), as well as observations taken at the Palomar Transient Factory in 2010, which gave an incorrect period solution of more than 9 hours ().

Satellite

During the photometric observation in 2005, it was revealed that Brorfelde is a binary asteroid. Its asteroid moon has an orbital period of hours, and measures approximately 1 kilometer in diameter, based on a mean-diameter ratio of for the system's secondary and primary body. In January 2014, repeated observations by Brian Warner confirmed a period of 2.503 and 18.51 hours for the primary and secondary, respectively (), with several online-published lightcurve plots.

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Brorfelde measures 3.78 kilometers in diameter, and its surface has an albedo of 0.46 (most recent result only). The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2747 and a diameter of 3.91 kilometers with an absolute magnitude of 14.062.

Naming

This minor planet was named on the occasion of the Brorfelde Observatory's 40th anniversary. Brorfelde was the observatory's first minor planet discovery. The approved naming citation was published by the Minor Planet Center on 7 September 1987 (M.P.C. 12210).

Notes

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 3309 Brorfelde — 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