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48 Doris

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
background#D6D6D6
name48 Doris
image48 Doris VLT (2021), deconvolved.pdf
discovererHermann Mayer Salomon Goldschmidt
discovered19 September 1857
pronounced
mpc_name(48) Doris
adjectivesDorian
named_afterDoris
mp_categoryMain belt
orbit_ref{{cite web
type2008-06-13 last obs
titleJPL Small-Body Database Browser: 48 Doris
urlhttps://ssd.jpl.nasa.gov/sbdb.cgi?sstr=48
access-date2008-11-10}}
epoch31 December 2006 (JD 2454100.5)
semimajor465.278 million km (3.110 AU)
perihelion430.463 million km (2.877 AU)
aphelion500.093 million km (3.343 AU)
eccentricity0.075
period2003.453 d (5.49 a)
inclination6.554°
asc_node183.754°
arg_peri257.583°
mean_anomaly336.191°
dimensions
flattening0.28
mean_diameter
(IRAS)
mass
density
rotation11.89 h
spectral_typeC
abs_magnitude7.14
albedo0.066

|access-date=2008-11-10}} (IRAS)

48 Doris is one of the largest main belt asteroids. It was discovered on 19 September 1857 by Hermann Goldschmidt from his balcony in Paris.

To find a name for the object, Jacques Babinet of the Academy of Sciences created a shortlist and asked the geologist Élie de Beaumont to make the selection. De Beaumont chose Doris, after an Oceanid in Greek mythology. Since Doris was discovered on the same night as 49 Pales, de Beaumont suggested naming the two "The Twins".

Physical characteristics

An occultation on 19 March 1981 suggested a diameter of 219±25 km.{{cite web |access-date=2008-12-07}} Observations of an occultation on 14 October 1999, using four well-placed chords, indicate an ellipsoid of 278×142 km and that 48 Doris is an extremely irregularly shaped object.{{cite web |access-date=2008-11-30 |archive-date=19 February 2012 |archive-url=https://web.archive.org/web/20120219025548/http://occsec.wellington.net.nz/planet/2001/plnres01.htm#Doris |url-status=dead

Doris will pass within 0.019 AU of Pallas in June 2132.{{cite web |access-date=2010-02-23}}

Notes

References

References

  1. {{MW. Doris
  2. {{OED. Dorian
  3. P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. ''Astronomy & Astrophysics'' 54, A56

  4. {{val. 2.12. 1.07. link. (2011-06-04 - Yu. Chernetenko, O. Kochetova, and V. Shor
    Kochetova (2004))
  5. Schmadel, Lutz D.. (2003). "Dictionary of Minor Planet Names". Springer Science & Business Media.
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