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3325 TARDIS

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name3325 TARDIS
background#D6D6D6
image003325-asteroid shape model (3325) TARDIS.png
captionShape model of TARDIS from its lightcurve
discovery_ref
discovered3 May 1984
discovererB. A. Skiff
discovery_siteAnderson Mesa Stn.
mpc_name(3325) TARDIS
alt_names1984 JZ
named_afterTARDIS
(fictional time and space machine)
mp_categorymain-belt(outer)
Alauda
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc58.56 yr (21,390 days)
aphelion3.2299 AU
perihelion3.1397 AU
semimajor3.1848 AU
eccentricity0.0142
period5.68 yr (2,076 days)
mean_anomaly45.895°
mean_motion/ day
inclination22.221°
asc_node46.246°
arg_peri86.099°
mean_diameter
(IRAS:9)
albedo(IRAS:9)
abs_magnitude11.5

(fictional time and space machine) Alauda (IRAS:9)

3325 TARDIS (provisional designation: ) is a dark Alauda asteroid from the outer region of the asteroid belt, approximately 29 km in diameter. It was discovered on 3 May 1984, by American astronomer Brian Skiff at Lowell's Anderson Mesa Station, Arizona, in the United States. The asteroid was named TARDIS, after the fictional time machine and spacecraft from the science fiction television series Doctor Who.

Orbit and classification

TARDIS is a member of the Alauda family (902), a large family of typically bright carbonaceous asteroids and named after its parent body, 702 Alauda.

It orbits the Sun in the outer main-belt at a distance of 3.1–3.2 AU once every 5 years and 8 months (2,076 days). Its orbit has an eccentricity of 0.01 and an inclination of 22° with respect to the ecliptic. In 1958 it was first identified as at the Goethe Link Observatory, extending the body's observation arc by 26 years prior to its official discovery at Anderson Mesa.

Naming

It is named after the acronym TARDIS (Time And Relative Dimension In Space), the space and time travel vehicle used by the Doctor in the British science fiction television series Doctor Who. The fictional time machine looks like a police telephone box from mid-twentieth century Britain. The official naming citation was published by the Minor Planet Center on 11 March 1990 (M.P.C. 16041).

Physical characteristics

According to the survey carried out by the Infrared Astronomical Satellite IRAS and NASA's NEOWISE mission, TARDIS measures 28.2 and 29.7 kilometers in diameter, and its surface has a low albedo of 0.055 and 0.067, respectively. An albedo between 0.05 and 0.06 is typical for carbonaceous asteroids of the outer main-belt. As of 2016, no rotational lightcurves have been obtained and the asteroid's period and shape still remains unknown.

References

|archive-url = https://web.archive.org/web/20200109120746/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2003325 |url-status = dead |archive-date = 9 January 2020 |access-date = 17 June 2017}}

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|access-date= 22 October 2019}}

|access-date = 1 March 2016}}

|access-date = 21 May 2016}}

|display-authors = 6

|access-date = 26 October 2019}}

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.

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