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

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

2672 Písek

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name2672 Písek
background#D6D6D6
discovery_ref
discovererJ. Kveton
discovery_siteKleť Obs.
discovered31 May 1979
mpc_name(2672) Písek
alt_names1979 KC1937 NP
named_afterPísek (Czech town)
mp_categorymain-belt(middle)
Eunomia
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc64.64 yr (23,609 d)
aphelion3.0006 AU
perihelion2.2257 AU
semimajor2.6132 AU
eccentricity0.1483
period4.22 yr (1,543 d)
mean_anomaly44.692°
mean_motion/ day
inclination14.139°
asc_node129.02°
arg_peri152.35°
mean_diameter
rotation
albedo
spectral_typeS (assumed)
abs_magnitude11.70
12.20
12.4
12.41

Eunomia

12.20 12.4 12.41

2672 Písek, provisional designation **, is a Eunomia asteroid from the central regions of the asteroid belt, approximately 25 km in diameter. It was discovered on 31 May 1979, by Yugoslav astronomer Jaroslav Květoň at the Kleť Observatory in the Czech Republic. The likely elongated asteroid is a suspected tumbler and a slow rotator with an exceptionally long period of 831 hours. It was named after the Czech town of Písek.

Orbit and classification

Písek is a core member of the Eunomia family (502), a prominent family of stony S-type asteroid and the largest one in the intermediate main belt with more than 5,000 members. It orbits the Sun in the central main-belt at a distance of 2.2–3.0 AU once every 4 years and 3 months (1,543 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.15 and an inclination of 14° with respect to the ecliptic.

The asteroid was first observed as ** at Johannesburg Observatory in July 1937. The body's observation arc begins with its observation as ** at Goethe Link Observatory in March 1953, more than 26 years prior to its official discovery observation at Klet.

Naming

This minor planet was named after the Czech town of Písek, located in the western South Bohemian Region known for its many prolific Czech writers and artists. The official naming citation was published by the Minor Planet Center on 28 January 1983 (M.P.C. 7620).

Physical characteristics

Písek is an assumed S-type asteroid, which agrees with the overall spectral type for members of the Eunomia family. Conversely, the space-based surveys found an albedo that is typical for a carbonaceous C-type or potentially darker D- and P-type asteroid (see below).

Rotation period

Between May and July 2017, a rotational lightcurve of Písek was obtained from photometric observations by Vladimir Benishek at Belgrade Astronomical Observatory in Serbia. Lightcurve analysis gave a rotation period of hours with a high brightness amplitude of 0.90 magnitude, indicative of a non-spherical shape ().

Diameter and albedo

According to the survey carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Písek measures between 20.18 and 29.60 kilometers in diameter and its surface has an albedo between 0.0294 and 0.091.

The Collaborative Asteroid Lightcurve Link assumes a standard albedo of 0.21 – derived from 15 Eunomia, the parent body of the Eunomia family– and consequently calculates a much smaller diameter of 9.60 kilometers based on an absolute magnitude of 12.4.

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 2672 Písek — 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