898 Hildegard

898 Hildegard /ˈhɪldɪɡɑːrd/ is a bright background asteroid, approximately 12 kilometers (7.5 miles) in diameter, that is located in the central regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 3 August 1918 and given the provisional designations A918 PG and 1918 EA.[1] The stony S-type asteroid (Sl) has a rotation period of 24.9 hours and a relatively high orbital eccentricity of 0.37. It was probably named after Saint Hildegard of Bingen (1098–1179).[3]

898 Hildegard
Modelled shape of Hildegard from its lightcurve
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date3 August 1918
Designations
(898) Hildegard
Pronunciation/ˈhɪldɪɡɑːrd/[2]
Named after
Hildegard of Bingen
(medieval abbess)[3]
A918 PG · 1936 PA
1918 EA
Orbital characteristics [4]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc101.51 yr (37,075 d)
Aphelion3.7448 AU
Perihelion1.7165 AU
2.7306 AU
Eccentricity0.3714
4.51 yr (1,648 d)
217.55°
0° 13m 6.24s / day
Inclination10.086°
241.55°
49.860°
Physical characteristics
Mean diameter
11.693±0.153 km[7]
24.855±0.002 h[8]
  • (344.0°, 27.0°) (λ1/β1)[6]
  • (164.0°, 8.0°) (λ2/β2)[6]
0.205±0.041[7]
SMASS = Sl [4]
11.7[1][4]

    Orbit and classification

    Hildegard is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[5][6] It orbits the Sun in the central asteroid belt at a distance of 1.7–3.7 AU once every 4 years and 6 months (1,648 days; semi-major axis of 2.73 AU). Its orbit has a high eccentricity of 0.37 and an inclination of 10° with respect to the ecliptic.[4] With a perihelion of 1.72 AU, Hildegard is notably close of becoming an outer-grazer to Mars, which has its aphelion at 1.67 AU. The body's observation arc begins at Heidelberg Observatory with its official discovery observation on 3 August 1918.[1]

    Naming

    This minor planet was probably named after Saint Hildegard of Bingen (1098–1179). The Benedictine abbess is considered to be the founder of scientific natural history in Germany. The naming was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 87).[3]

    Physical characteristics

    In the Bus–Binzel SMASS classification, Hildegard is an Sl-subtype, which transitions from the common stony S-type to the uncommon L-type asteroid.[4][6]

    Rotation period

    In April 2008, a rotational lightcurve of Hildegard was obtained from photometric observations by Australian amateur astronomer David Higgins. Lightcurve analysis gave a well-defined rotation period of 24.855±0.002 hours with a brightness variation of 0.36±0.01 magnitude (U=3).[8] Previously in June 1999, observations by Brian Warner at his Palmer Divide Observatory (716) in Colorado only gave a period of above 24 hours and an amplitude larger than 0.3 magnitude (U=1).[9][lower-alpha 1] Asteroid's with a rotation period near 24 hours are difficult to observe, since full coverage can not be obtained by a few consecutive nights of observation from a single observatory alone, due to Earth's nearly synchronous rotation. In such cases, international collaborations are highly useful with each observatory covering a different section of the lightcurve.

    In 2016, a modeled lightcurve gave a concurring sidereal period of 24.8544±0.0005 hours using data from a large collaboration of individual observers (such as above). The study also determined two spin axes of (344.0°, 27.0°) and (164.0°, 8.0°) in ecliptic coordinates (λ, β).[10]

    Diameter and albedo

    According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Hildegard measures 11.693±0.153 kilometers in diameter and its surface has an albedo of 0.205±0.041.[6][7] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 13.58 kilometers based on an absolute magnitude of 11.7.[8]

    Notes
    1. Lightcurve plot of (898) Hildegard, Palmer Divide Observatory, Brian Warner (1999). Rotation period larger than 24 hours with a brightness amplitude larger than 0.3 mag. Quality code is 1. Summary figures at the LCDB.
    gollark: It uses porter stemming to normalize "bee" and "bees" into "bee".
    gollark: Anyway, SQLite documents it, but the basic idea is that you have a table like this```sqlCREATE TABLE thing ( token TEXT NOT NULL, document_id INTEGER NOT NULL);```so when you look up "bees" it searches for the token "bees" in there using an index and retrieves the resulting document.
    gollark: [REDACTED].
    gollark: FTS5 uses inverted index™ technology.
    gollark: Yep! It has to linear-scan through all rows of the database to check.

    References
    1. "898 Hildegard (A918 PG)". Minor Planet Center. Retrieved 24 February 2020.
    2. "Hildegard". Dictionary.com Unabridged. Random House.
    3. Schmadel, Lutz D. (2007). "(898) Hildegard". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 81. doi:10.1007/978-3-540-29925-7_899. ISBN 978-3-540-00238-3.
    4. "JPL Small-Body Database Browser: 898 Hildegard (A918 PG)" (2020-02-04 last obs.). Jet Propulsion Laboratory. Retrieved 24 February 2020.
    5. "Asteroid 898 Hildegard – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 24 February 2020.
    6. "Asteroid 898 Hildegard". Small Bodies Data Ferret. Retrieved 24 February 2020.
    7. Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68.
    8. "LCDB Data for (898) Hildegard". Asteroid Lightcurve Database (LCDB). Retrieved 24 February 2020.
    9. Warner, B. D. (December 1999). "Asteroid Photometry at the Palmer Divide Observatory" (PDF). Minor Planet Bulletin. 26 (4): 31. Bibcode:1999MPBu...26...31W.
    10. Hanuš, J.; Ďurech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network". Astronomy and Astrophysics. 586: A108. arXiv:1510.07422. Bibcode:2016A&A...586A.108H. doi:10.1051/0004-6361/201527441. ISSN 0004-6361.
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