735 Marghanna

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735 Marghanna
Discovery [1]
Discovered byH. Vogt
Discovery siteHeidelberg Obs.
Discovery date9 December 1912
Designations
(735) Marghanna
Named after
Margarete Vogt [2]
and Hanna
(discoverer's mother/relative)
A912 XD · 1952 OH
1952 OJ · 1952 QA
1952 QB · 1912 PY
Perihelion
1.8535 AU
2.7297 AU
Eccentricity0.3210
4.51 yr (1,647 d)
346.73°
0° 13m 6.6s / day
Inclination16.866°
42.952°
309.76°
Physical characteristics
Mean diameter
  • 67.235±0.513 km[7]
  • 74.32±1.6 km[8]
  • 78.69±1.62 km[9]
Synodic rotation period
20.625±0.011 h[11]
  • 0.043±0.002[9]
  • 0.0484±0.0484[8]
  • 0.059±0.007[7]

735 Marghanna (

rotation period of 20.6 hours and is rather regular in shape. It was named after Margarete Vogt and after Hanna, the mother and a relative of the discoverer, respectively.[2]

Orbit and classification

Marghanna is a non-

Heidelberg Observatory on 29 November 1921, almost nine years after its official discovery observation.[1]

Naming

This

H 74).[2]

Physical characteristics

In the

SMASS classification, it is a hydrated C-type (Ch).[3][5][12]

Rotation period

In May 2011, a rotational

U=2/1+/3−).[15]

Diameter and albedo

According to the surveys carried out by the

albedo of (0.059±0.007), (0.0484±0.0484) and (0.043±0.002), respectively.[7][8][9]

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0423 and a diameter of 74.23 kilometers based on an absolute magnitude of 9.7,[15] while the Cornell Mid-IR Asteroid Spectroscopy (MIDAS) survey determined a diameter of (73±6) kilometers and Benoit Carry one of (72.27±2.22) kilometers.[10][16] Alternative mean-diameters published by the WISE team include (57.25±26.07 km), (67.976±0.404 km), (70.640±1.230 km) and (87.951±34.60 km) with a corresponding albedo of (0.05±0.09), (0.059±0.007), (0.0536±0.0078) and (0.0275±0.0259).[5][15]

Two

asteroid occultations on 11 March 2008 and on 4 May 2010, gave a best-fit ellipse dimension of (81.6 km × 73.5 km) and (74.0 km × 64.0 km), respectively, each with an intermediate quality rating of 2.[5] These timed observations are taken when the asteroid passes in front of a distant star.[5]

References

  1. ^ a b c d e "735 Marghanna (A912 XD)". Minor Planet Center. Retrieved 9 June 2020.
  2. ^
    ISBN 978-3-540-00238-3
    .
  3. ^ a b c d e f g h i "JPL Small-Body Database Browser: 735 Marghanna (A912 XD)" (2020-04-28 last obs.). Jet Propulsion Laboratory. Retrieved 9 June 2020.
  4. ^ a b "Asteroid 735 Marghanna – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 9 June 2020.
  5. ^ a b c d e f "Asteroid 735 Marghanna". Small Bodies Data Ferret. Retrieved 9 June 2020.
  6. ^ a b Zappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997). "Asteroid Dynamical Families". NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. Retrieved 9 June 2020.} (PDS main page)
  7. ^
    Bibcode:2016PDSS..247.....M
    . Retrieved 9 June 2020.
  8. ^
    Bibcode:2004PDSS...12.....T
    . Retrieved 9 June 2020.
  9. ^
    doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153
    )
  10. ^
    doi:10.1016/j.pss.2012.03.009
    . See Table 1.
  11. ^
    ISSN 1052-8091
    .
  12. ^
    doi:10.1051/0004-6361/200913322. Retrieved 9 June 2020. (PDS data set)
  13. ISSN 0004-6256
    .
  14. ^ Behrend, Raoul. "Asteroids and comets rotation curves – (735) Marghanna". Geneva Observatory. Retrieved 9 June 2020.
  15. ^ a b c "LCDB Data for (735) Marghanna". Asteroid Lightcurve Database (LCDB). Retrieved 9 June 2020.
  16. ISSN 0019-1035
    .

External links
Retrieved from "https://en.wikipedia.org/w/index.php?title=735_Marghanna&oldid=1190800604"