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1657 Roemera

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1657 Roemera
Discovery [1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date6 March 1961
Designations
1657 Roemera
Named after
Elizabeth Roemer
(astronomer)[2]
1961 EA · 1932 AB
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 27 June 2015 (JD 2457200.5)
Uncertainty parameter 0
Observation arc83.43 yr (30,473 days)
Aphelion2.9031 AU
Perihelion1.7933 AU
2.3482 AU
Eccentricity0.2363
3.60 yr (1,314 days)
34.334°
Inclination23.376°
105.33°
54.332°
Earth MOID0.8808 AU
Physical characteristics
Dimensions7.67±0.22 km[4]
8.04 km (caculated)[3]
34.0 h[5]
4.5±1 h[6]
0.220±0.030[4]
0.20 (assumed)[3]
Tholen = S
S[3]
12.84

1657 Roemera, provisional designation 1961 EA, is a stony asteroid from the inner regions of the asteroid belt, about 8 kilometers in diameter. It was discovered by astronomer Paul Wild at Zimmerwald Observatory near Bern, Switzerland on 6 March 1961.[7]

The asteroid orbits the Sun at a distance of 1.8–2.9 AU once every 3.6 years (1,314 days). Its orbit shows an eccentricity of 0.24 and is tilted by 23 degrees to the plane of the ecliptic. The S-type asteroid has a long rotation period of 34 hours[5] and a relatively high albedo of 0.22.[4]

It was named by the discoverer in honor American female astronomer Elizabeth Roemer (b. 1929), U.S. Naval Observatory, in appreciation of her untiring and successful efforts to advance the knowledge of the motions and physical properties of comets and minor planets.[2] Roemer herself discovered the asteroids 1930 Lucifer and 1983 Bok.

References

  1. ^ a b "JPL Small-Body Database Browser: 1657 Roemera (1961 EA)" (2015-06-16 last obs.). Jet Propulsion Laboratory. Retrieved November 2015. {{cite web}}: Check date values in: |accessdate= (help)
  2. ^ a b Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1657) Roemera. Springer Berlin Heidelberg. p. 132. ISBN 978-3-540-29925-7. Retrieved November 2015. {{cite book}}: Check date values in: |accessdate= (help)
  3. ^ a b c d "LCDB Data for (1657) Roemera". Asteroid Lightcurve Database (LCDB). Retrieved November 2015. {{cite web}}: Check date values in: |accessdate= (help)
  4. ^ a b c Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved November 2015. {{cite journal}}: Check date values in: |access-date= (help)
  5. ^ a b Warner, Brian D. (January 2009). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 May - September". Bulletin of the Minor Planets. 36 (1). Section of the Association of Lunar and Planetary Observers: 7–13. Bibcode:2009MPBu...36....7W. ISSN 1052-8091. Retrieved November 2015. {{cite journal}}: Check date values in: |access-date= (help)
  6. ^ Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids". Abstracts of the Lunar and Planetary Science Conference. Bibcode:1995LPI....26.1511W. Retrieved November 2015. {{cite journal}}: Check date values in: |access-date= (help)
  7. ^ "1657 Roemera (1961 EA)". Minor Planet Center. Retrieved November 2015. {{cite web}}: Check date values in: |accessdate= (help)