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1122 Neith
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Main-belt asteroid
July 2020
yes
1122 Neith
#D6D6D6
E. Delporte
Uccle Obs.
17 September 1928
(1122) Neith
1928 SB1941 YH1953 OAA924 VA
' n iː ɪ θ
Neith (Egyptian mythology)
main-belt(middle)background
4 September 2017 (JD 2458000.5)
0
93.01 yr (33,971 days)
3.2763 AU
1.9347 AU
2.6055 AU
0.2575
4.21 yr (1,536 days)
30.680°
0.2343 ms / day
4.7381°
63.385°
328.96°
11.566 0.261 km11.73 km (derived)12.01 0.5 km13.453 1.632 km13.81 0.73 km13.84 1.46 km (MSX)34
12.599 0.006 h
0.206 0.0480.2756 (derived)0.2836 0.04350.284 0.0430.340.4450 0.044
AS (assumed)
11.1011.6711.711.71 0.4911.9
1122 Neith ' n iː ɪ θ,that is, pronounced with two syllables, NEE-ith. provisional designation 1928 SB, is a background asteroid from the central region of the asteroid belt, approximately 12 kilometers in diameter. It was discovered by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle on 17 September 1928. The asteroid was named after the goddess Neith from Egyptian mythology.
Orbit and classification
Neith is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 1.9–3.3 AU once every 4 years and 3 months (1,536 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.26 and an inclination of 5° with respect to the ecliptic. The body's observation arc begins with its observation as A924 VA at Heidelberg Observatory in November 1924, almost four years prior to its official discovery observation at Uccle.
Physical characteristics
Neith has been characterized as an uncommon A-type asteroid during a spectroscopic survey after it had previously been classified as X-type in the Tholen taxonomy. The asteroid's surface shows a strong 0.96 μm absorption band (depth of 24%) and a steep slope in the near-infrared region, typical of olivine-rich bodies. The survey was conducted at the NTT, TNG and IRTF telescopes during 2004–2007.
Rotation period
In September 2008, a rotational lightcurve of Neith was obtained from photometric observations by Julian Oey at the Leura and Kingsgrove Observatory in Australia. Lightcurve analysis gave a synodic rotation period of 12.5990 hours with a brightness variation of 0.08 magnitude (U=2).
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS (SIMPS and MSX), the Spitzer Space Telescope (MIPS photometer and MIPSGAL survey) and the NEOWISE mission of the Wide-field Infrared Survey Explorer, Neith measures between 11.566 and 13.84 kilometers in diameter and its surface has an albedo between 0.206 and 0.4450.34
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2756 and a diameter of 11.73 kilometers based on an absolute magnitude of 11.67.
Naming
This minor planet was named from Egyptian mythology after the goddess of Libyan origin, Neith, goddess of the hunt and of war, believed to be the mother of the Sun. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 105).
References
30em 2017-11-27 last obs.
JPL Small-Body Database Browser: 1122 Neith (1928 SB)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001122
Jet Propulsion Laboratory
25 January 2018
Dictionary of Minor Planet Names – (1122) Neith
Schmadel Lutz D.
Springer Berlin Heidelberg
95
2007
https://books.google.com/books?id=aeAg1X7afOoC&dq=1122+Neith&pg=PA94
978-3-540-00238-3
1122 Neith (1928 SB)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1122
25 January 2018
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
J. Dailey
P. R. M. Eisenhardt
R. S. McMillan
T. B. Spahr
M. F. Skrutskie
D. Tholen
R. G. Walker
E. L. Wright
E. DeBaun
D. Elsbury
T. IV Gautier
S. Gomillion
A. Wilkins
118745497 November 2011
Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters
The Astrophysical Journal
741
2
20
2011ApJ...741...68M
10.1088/0004-637X/741/2/68
1109.4096
6
Erin Lee Ryan
Donald R. Mizuno
Sachindev S. Shenoy
Charles E. Woodward
Sean Carey
Alberto Noriega-Crespo
Kathleen E. Kraemer
Stephan D. Price
April 2012
The Kilometer-Sized Main Belt Asteroid Population as Revealed by Spitzer
astro-ph.EP 1204.1116
Asteroid 1122 Neith – Proper Elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1122
28 October 2019
1122
25 January 2018
6
A. Mainzer
T. Grav
J. Masiero
E. Hand
J. Bauer
D. Tholen
R. S. McMillan
T. Spahr
R. M. Cutri
E. Wright
J. Watkins
W. Mo
C. Maleszewski
118700974 November 2011
NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407
E. F. Tedesco
P. V. Noah
M. Noah
S. D. Price
October 2004
IRAS Minor Planet Survey V6.0
https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
NASA Planetary Data System
12
IRAS-A-FPA-3-RDR-IMPS-V6.0
2004PDSS...12.....T
22 October 2019
6
E. L. Ryan
D. R. Mizuno
S. S. Shenoy
C. E. Woodward
S. J. Carey
A. Noriega-Crespo
K. E. Kraemer
S. D. Price
21069867 June 2015
The kilometer-sized Main Belt asteroid population revealed by Spitzer
Astronomy and Astrophysics
578
12
2015A&A...578A..42R
10.1051/0004-6361/201321375
1204.1116
Oey, Julian
October 2009
Lightcurve Analysis of Asteroids from Leura and Kingsgrove Observatory in the Second Half of 2008
The Minor Planet Bulletin
36
4
162–164
1052-8091
2009MPBu...36..162O
S. Fornasier
B. E. Clark
E. Dotto
118549118
July 2011
Spectroscopic survey of X-type asteroids
Icarus
214
1
131–146
2011Icar..214..131F
10.1016/j.icarus.2011.04.022
1105.3380
Gerard Faure
Lawrence Garrett
October 2009
Suggested Revised H Values of Selected Asteroids: Report Number 4
The Minor Planet Bulletin
36
4
140–143
1052-8091
2009MPBu...36..140F
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
53493339 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
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
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1122
1121 Natascha 1122 1123 Shapleya
001122
Category:Discoveries by Eugène Joseph Delporte
Category:Named minor planets
19280917