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1025 Riema
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Asteroid
October 2019
yes
1025 Riema
#D6D6D6
12 August 1923
K. Reinmuth
Heidelberg Obs.
(1025) Riema
1923 NXA923 QA
Johannes Riem(German astronomer)
main-belt(inner)Hungaria
4 September 2017 (JD 2458000.5)
0
93.81 yr (34,264 days)
2.0572 AU
1.9009 AU
1.9790 AU
0.0395
2.78 yr (1,017 days)
102.31°
0.3540 ms / day
26.863°
163.39°
349.06°
4.605 0.171 km5.48 km (derived)
3.566 0.005 h3.578 0.002 hlcdb-Warner-2017lightcurveplot-PDS3.580 0.005 h3.581 0.002 hlightcurveplot-PDO3.581 0.001 hlightcurveplot-PDS3.588 0.002 hlightcurveplot-PDS6.557 0.001 h
1.000 0.0000.166 0.0360.40 (assumed)
E (Tholen), Xe (SMASS)MXeB–V = 0.714U–B = 0.294V–R = 0.440 0.010
12.3012.512.57 0.2812.92 0.04
1025 Riema, provisional designation 1923 NX, is a bright Hungaria asteroid from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 12 August 1923, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The asteroid was named after ARI astronomer Johannes Riem.
Orbit and classification
Riema is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun at a distance of 1.9–2.1 AU once every 2 years and 9 months (1,017 days). Its orbit has an eccentricity of 0.04 and an inclination of 27° with respect to the ecliptic. The asteroid's observation arc begins at Heidelberg, four nights after its official discovery observation.
Physical characteristics
In the Tholen classification, Riema is a bright E-type asteroid. In the SMASS taxonomy, it has been classified as a Xe-type, which transitions from the E to the X-types. In addition, the asteroid has also been polarimetrically characterized as a metallic M-type asteroid.
Lightcurves
In August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2).
The Ukrainian team also determined the body's poles and axis-ratios. They found a spin axis of (141.0°, 11.0°) and (321.0.0°, −13.0°) in ecliptic coordinates (λ, β), as well as a semi-axis ratio of 3.41 (a/b) and 1.16 (b/c) for the three-axial ellipsoid model (Q=2).
Between 2003 and 2017, several additional lightcurves were obtained by American photometrists Robert Stephens and Brian Warner at the Santana Observatory (646), the Palmer Divide Observatory (716) and the Palmer Divide Station (U82), respectively. The constructed lightcurve gave a shorter period for Riema between 3.566 and 3.588 hours with a low amplitude of 0.06 to 0.19 magnitude (U=2/2/2+/2+/3/3).lcdb-Warner-2017lightcurveplot-PDOlightcurveplot-PDS
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Riema measures 4.605 kilometers in diameter and its surface has an outstandingly high albedo of 1.000. The Collaborative Asteroid Lightcurve Link assumes an albedo for E-type Hungaria asteroids of 0.40 – taken from 434 Hungaria, the family's largest member and namesake – and derives a diameter of 5.48 kilometers based on an absolute magnitude of 12.92.
Naming
This minor planet was named after Johannes Karl Richard Riem (1868–1945), a German astronomer at the Astronomisches Rechen-Institut (ARI) in Berlin. The name was suggested by ARI. The official naming citation was published by Paul Herget in The Names of the Minor Planets in 1955 (H 98).
Notes
lightcurveplot-PDO Lightcurve plot of 1025 Riema with a period of 3.581 0.002 hours, Palmer Divide Observatory, Colorado, B. D. Warner (2012)
lcdb-Warner-2017 Warner (2017) web: rotation period 3.578 0.002 hours with a brightness amplitude of 0.06 mag. Summary figures for (1025) Riema at Collaborative Asteroid Lightcurve Link (CALL)
lightcurveplot-PDS Lightcurve plots by B. D. Warner at the Palmer Divide Station in California:
(2014), (2015) and (2017)
References
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Jet Propulsion Laboratory
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Dictionary of Minor Planet Names – (1025) Riema
Schmadel Lutz D.
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88
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1025 Riema (1923 NX)
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6 July 2017
Spratt, Christopher E.
April 1990
The Hungaria group of minor planets
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123–131
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1025
6 July 2017
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Joseph R. Masiero
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T. Grav
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V. G. Shevchenko
Yu. N. Krugly
V. G. Chiorny
I. N. Belskaya
N. M. Gaftonyuk
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Rotation and photometric properties of E-type asteroids
https://www.researchgate.net/publication/222944146
Planetary and Space Science
51
9–10
525–532
2003P&SS...51..525S
10.1016/S0032-0633(03)00076-X
6 July 2017
Stephens, Robert D.
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30
4
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Warner, Brian D.
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Warner, Brian D.
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Warner, Brian D.
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3
144–155
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Warner, Brian D.
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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
1025
1024 Hale 1025 1026 Ingrid
001025
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
001025
001025
19230812