1711 Sandrine

1711 Sandrine, provisional designation 1935 BB, is a stony Eoan asteroid from the outer region of the asteroid belt, approximately 23 kilometers in diameter.

1711 Sandrine
Discovery [1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date29 January 1935
Designations
(1711) Sandrine
Named after
(grand-nice of astronomer)
Georges Roland[2]
1935 BB · 1938 SF1
1943 QE · 1949 WF
1951 CX1 · 1952 HG1
1956 AH · 1956 AW
1956 DC · 1959 TR
1959 UH · A909 DJ
main-belt · (outer)
Eos [3]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc107.82 yr (39,380 days)
Aphelion3.3596 AU
Perihelion2.6666 AU
3.0131 AU
Eccentricity0.1150
5.23 yr (1,910 days)
5.6639°
0° 11m 18.24s / day
Inclination11.095°
134.78°
251.25°
Physical characteristics
Dimensions22.929±0.364 km[4]
0.133±0.011[4]
Tholen = S [1]
B–V = 0.855[1]
U–B = 0.447[1]
11.01[1]

    This asteroid was discovered on 29 January 1935, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle.[5] It was named after the grand-nice of astronomer Georges Roland.[2]

    Classification and orbit

    Sandrine is a member of the Eos family (606), the largest asteroid family in the outer main belt consisting of nearly 10,000 asteroids.[3][6]:23 It orbits the Sun in the outer main-belt at a distance of 2.7–3.4 AU once every 5 years and 3 months (1,910 days). Its orbit has an eccentricity of 0.12 and an inclination of 11° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation. Its first observation at Heidelberg in 1909, when it was identified as A909 DJ, has been discarded.[5]

    Physical characteristics

    In the Tholen classification, Sandrine is characterized as a common S-type asteroid.[1]

    Diameter and albedo

    According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Sandrine measures 22.93 kilometers in diameter, and its surface has an albedo of 0.133.[4] It has an absolute magnitude of 11.01.[1]

    Lightcurves

    As of 2017, Sandrine's rotation period and shape remain unknown.[1]

    Naming

    This minor planet was named after Sandrine, a grand-niece of Georges Roland, astronomer at Uccle and co-discoverer of Comet Arend–Roland. Delporte also named 1707 Chantal and 1848 Delvaux after family members of his collaborator.[2] The official naming citation was published by the Minor Planet Center on 8 April 1982 (M.P.C. 6832).[7]

    gollark: Also seems to be the trade hub rule attitude.
    gollark: "I don't X. Therefore thing-related-to-X is unnecessary"
    gollark: I can't think of other explanations for its current management.
    gollark: Well, it could be part of the drama maximisation plan...
    gollark: After that. TJ09 never forgave him.

    References
    1. "JPL Small-Body Database Browser: 1711 Sandrine (1935 BB)" (2016-12-13 last obs.). Jet Propulsion Laboratory. Retrieved 7 June 2017.
    2. Schmadel, Lutz D. (2007). "(1711) Sandrine". Dictionary of Minor Planet Names – (1711) Sandrine. Springer Berlin Heidelberg. p. 136. doi:10.1007/978-3-540-29925-7_1712. ISBN 978-3-540-00238-3.
    3. "Asteroid 1711 Sandrine – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
    4. Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. Retrieved 18 December 2016.
    5. "1711 Sandrine (1935 BB)". Minor Planet Center. Retrieved 18 December 2016.
    6. Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). Identification and Dynamical Properties of Asteroid Families. Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
    7. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 18 December 2016.

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