411 REFERENCE · Wikipedia
(7025) 1993 QA
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Sub-kilometer asteroid classified as a near-Earth object
October 2019
yes
(7025) 1993 QA
#FFC2E0
Spacewatch
Kitt Peak National Obs.
16 August 1993
(7025) 1993 QA
NEOApolloAmor
4 September 2017 (JD 2458000.5)
0
22.88 yr (8,358 days)
1.9405 AU
1.0111 AU
1.4758 AU
0.3149
1.79 yr (655 days)
25.431°
0.5498 ms / day
12.607°
146.64°
323.39°
0.0645 AU25.1 LD
0.498 0.171 km0.77 km (derived)
2.5057 h
0.20 (assumed)0.340 0.234
DS
17.9418.0018.318.75 0.47
(7025) 1993 QA is a sub-kilometer asteroid classified as a near-Earth object of the Apollo and Amor group, respectively. It was discovered on 16 August 1993, by astronomers of the Spacewatch program at the Kitt Peak National Observatory near Tucson, Arizona, United States. The asteroid measures approximately half a kilometer in diameter and has a short rotation period of 2.5057 hours.
Orbit and classification
1993 QA is a member of the dynamical Apollo group, which are Earth-crossing asteroids. Conversely, it is classified as a non-Earth crossing Amor asteroid by the Minor Planet Center, due to its near-threshold perihelion of 1.011 AU.
It orbits the Sun at a distance of 1.01–1.94 AU once every 21 months (655 days; semi-major axis of 1.48 AU). Its orbit has an eccentricity of 0.31 and an inclination of 13° with respect to the ecliptic. The body's observation arc begins with its official discovery observation by Spacewatch on 16 August 1993.
Close approaches
The asteroid has an Earth minimum orbital intersection distance of 0.0645 AU km on on 3, which translates into 25.1 lunar distances. On 6 February 1996 it transited Earth at a nominal distance of 0.07080 AU km mi on off 3 flip. The body's next encounter with Earth below 0.1 AU will occur on 24 January 2025, at a distance of 0.06275 AU km mi on off 3 flip.
Physical characteristics
1993 QA has been characterized as a dark D-type asteroid on images taken by the Sloan Digital Sky Survey. Conversely, Pan-STARRS photometric survey determined a much brighter S-type.
Rotation period
In the late 1990s, two rotational lightcurves of 1993 QA were obtained from photometric observations by European astronomers. Lightcurve analysis gave an identical, well-defined rotation period of 2.5057 hours with a brightness amplitude of 0.32 and 0.50 magnitude, respectively (U=3/3). Its period is near the cohesionless spin-barrier of 2.2 hours, which set the upper limit for fast-rotating asteroids.
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, 1993 QA measures 498 meters in diameter and its surface has a high albedo of 0.340. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 770 meters based on an absolute magnitude of 17.94.
Naming
As of 2018, this minor planet has not been named yet.
References
30em 2016-07-04 last obs.
JPL Small-Body Database Browser: 7025 (1993 QA)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2007025
Jet Propulsion Laboratory
25 January 2018
7025 (1993 QA)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=7025
25 January 2018
7025
25 January 2018
6
C. R. Nugent
A. Mainzer
J. Masiero
J. Bauer
R. M. Cutri
T. Grav
E. Kramer
S. Sonnett
R. Stevenson
E. L. Wright
December 2015
NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos
The Astrophysical Journal
814
2
13
2015ApJ...814..117N
10.1088/0004-637X/814/2/117
1509.02522
9341381
Petr Pravec
Marek Wolf
Lenka Sarounová
November 1998
Lightcurves of 26 Near-Earth Asteroids
Icarus
136
1
124–153
1998Icar..136..124P
10.1006/icar.1998.5993
6
Yu. N. Krugly
I. N. Belskaya
V. G. Shevchenko
V. G. Chiorny
F. P. Velichko
S. Mottola
A. Erikson
G. Hahn
A. Nathues
G. Neukum
N. M. Gaftonyuk
E. Dotto
August 2002
The Near-Earth Objects Follow-up Program. IV. CCD Photometry in 1996-1999
Icarus
158
2
294–304
2002Icar..158..294K
10.1006/icar.2002.6884
B. Carry
E. Solano
S. Eggl
F. E. DeMeo
April 2016
Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry
Icarus
268
340–354
2016Icar..268..340C
10.1016/j.icarus.2015.12.047
1601.02087
119258489
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
Christopher Waters
November 2015
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
Icarus
261
34–47
2015Icar..261...34V
10.1016/j.icarus.2015.08.007
1506.00762
53493339
External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
7025
7025 1993QA
7025
007025
007025
007025
19930816