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

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

1696 Nurmela

Baptistina asteroid


Baptistina asteroid

FieldValue
minorplanetyes
name1696 Nurmela
background#D6D6D6
discovery_ref
discovered18 March 1939
discovererY. Väisälä
discovery_siteTurku Obs.
mpc_name(1696) Nurmela
alt_names1939 FF1939 GL
1949 DK1951 YK
named_afterTauno Nurmela
(University of Turku)
mp_categorymain-beltinner
BaptistinaFlora
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc78.30 yr (28,598 d)
aphelion2.4842 AU
perihelion2.0391 AU
semimajor2.2616 AU
eccentricity0.0984
period3.40 yr (1,242 d)
mean_anomaly76.752°
mean_motion/ day
inclination6.0374°
asc_node21.035°
arg_peri164.84°
mean_diameter
(calculated)
rotation
albedo(assumed)
spectral_typeC (assumed)
abs_magnitude12.90
13.19

1949 DK1951 YK (University of Turku) BaptistinaFlora

(calculated)

13.19

1696 Nurmela, provisional designation , is a Baptistina asteroid from the inner regions of the asteroid belt, approximately 10 km in diameter. It was discovered on 18 March 1939, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland, and named after Finnish academician Tauno Nurmela. The possibly elongated asteroid has a rotation period of 3.15 hours.

Orbit and classification

Nurmela is the second-largest member of the small Baptistina family (403), a large inner-belt family, named after 298 Baptistina, its largest member and namesake. When applying the hierarchical clustering method to its proper orbital elements, it is also 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 main-belt at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,242 days; semi-major axis of 2.26 AU). Its orbit has an eccentricity of 0.10 and an inclination of 6° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Turku.

Physical characteristics

Nurmela is an assumed carbonaceous C-type asteroid, while its albedo and membership to the Baptistina family is indicative for an X-type.

Rotation period

In March and April 2007, two rotational lightcurves of Nurmela was obtained from photometric observations by Adrián Galád and Robert Stephens. They gave an identical rotation period of 3.1587 hours with a brightness variation of 0.33 and 0.42 magnitude, respectively (). In April 2017, another observation by Stephens gave a concurring period of 3.159 hours () with an amplitude of 0.58 magnitude, indicative for an elongated shape.

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Nurmela measures between 6.06 and 10.31 kilometers in diameter and its surface has an albedo between 0.116 and 0.28.

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 14.64 kilometers based on an absolute magnitude of 12.9.

Naming

This minor planet was named in honor of Finnish academician Tauno Kalervo Nurmela (1907–1985), some time professor of Romanic philology and later chancellor of University of Turku. The official naming citation was published by the Minor Planet Center on 1 April 1980 (M.P.C. 5281).

Notes

References

|display-authors = 6

|display-authors = 6 |doi-access=

|display-authors = 6

|display-authors = 6

|display-authors = 6

|access-date= 17 December 2016}}

|access-date= 17 December 2016}}

|access-date= 10 November 2015}}

|access-date= 19 April 2018}}

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 1696 Nurmela — 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