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

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

997 Priska

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name997 Priska
background#D6D6D6
discovery_ref
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
discovered12 July 1923
mpc_name(997) Priska
alt_names1923 NR1959 WA
1967 RN
pronounced
named_afterA girl's name picked from a
popular German calendar
mp_categorymain-belt(middle)
Adeona
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc93.71 yr (34,229 days)
aphelion3.1568 AU
perihelion2.1787 AU
semimajor2.6677 AU
eccentricity0.1833
period4.36 yr (1,592 days)
mean_anomaly206.91°
mean_motion/ day
inclination10.508°
asc_node247.11°
arg_peri51.494°
dimensionskm
km
18.59 km (derived)
km
km
km
km
km
rotationh
albedo
0.0511 (derived)
spectral_typeSMASS Ch
abs_magnitude12.0012.4012.512.5113.07

1967 RN popular German calendar Adeona km 18.59 km (derived) km km km km km

0.0511 (derived)

997 Priska, provisional designation , is a carbonaceous Adeonian asteroid from the central regions of the asteroid belt, approximately 19 kilometers in diameter. It was discovered on 12 July 1923, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid's name is a common German female name, unrelated to the discoverer's contemporaries.

Orbit and classification

Priska is a member of the Adeona family (505), a large family of carbonaceous asteroids in the central main belt, named after 145 Adeona. It orbits the Sun at a distance of 2.2–3.2 AU once every 4 years and 4 months (1,592 days). Its orbit has an eccentricity of 0.18 and an inclination of 11° with respect to the ecliptic.

The body's observation arc begins with its official discovery observation at Heidelberg.

Physical characteristics

In the SMASS classification, Priska is a Ch-subtype, a hydrated carbonaceous C-type asteroid.

Rotation period

In August 2006, a rotational lightcurve of Priska was obtained from photometric observations by Italian amateur astronomers Roberto Crippa and Federico Manzini. Lightcurve analysis gave a rotation period of 16.22 hours with a brightness amplitude of 0.61 magnitude (). A high brightness variation is typically indicative for an elongated rather than spherical shape.

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Priska measures between 16.71 and 20.391 kilometers in diameter and its surface has an albedo between 0.037 and 0.088.

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0511 and a diameter of 18.59 kilometers based on an absolute magnitude of 12.5.

Naming

This minor planet was named after a girl's name picked from the German popular calendar Der Lahrer hinkende Bote.(de)

Reinmuth's ''Calendar Girls''

As with 913 Otila and 1144 Oda, Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries. The author of the Dictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.

References

References

  1. 'Prisca' in Noah Webster (1884) ''A Practical Dictionary of the English Language''
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 997 Priska — 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