In February 1995, using the Spacewatch telescope at the Kitt Peak
observatory, Jedicke (1995) discovered a very faint asteroid of an
absolute magnitude H=25 when it passed near the Earth at a
distance of about 2 million km. The equivalent diameter d of 1995 CS,
calculated using the following expression (Bowell & Lumme 1982)
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(4) |
The similarity in the directions of perihelion, semi-major axes,
eccentricity, and perihelion distances of these two objects imply that
they separated from a common body at an earlier time or the smaller 1995 CS
detached from the larger Adonis (Steel 1997). In order to investigate
possible genetic relationship of the Adonis and 1995 CS, Steel (1997)
performed a series of back integrations of the orbits of Adonis and
1995 CS over the time span of 55 000 yr and came to the conclusion that
these two objects might have had identical orbits at least
30 000 yr ago
and therefore:
1) the small asteroid 1995 CS may be a fragment of the larger body (2101) Adonis, which by then represented an extinct or dormant cometary nucleus, or
2) as for 1995 CS, Adonis is itself a fragment of a larger cometary body yet to be discovered, or that might be known but wandered into a sufficiently different orbit, or
3) it is possible that Adonis and 1995 CS do not share a common origin, but occupy similar orbits in the present epoch merely by chance.
Our back integration of the orbit of 1995 CS over
15 000 yr performed by the Halphen-Goryachev (Goryachev 1937) method
shows that 1995 CS is a quadruple-crosser of the Earth's orbit for the
same values of the argument of perihelion
as Adonis (Fig. 1).
Moreover, it was found that the orbital elements of 1995 CS coincide
nearly with the theoretical ones of day-time
-Capricornids (Table 1).
Therefore it seems that 1995 CS belongs to the meteoroid stream
associated with Adonis. At the time of its discovery, the
radius-vector of the ascending node of 1995 CS was equal to
1.0 AU, and so using 1995 CS' orbital elements, for the point of
minimum distance from the Earth's orbit we
calculated the theoretical geocentric radiant and velocity equal to:
The membership of 1995 CS to the day-time
-Capricornid meteor shower shows that meteoroid streams may be
populated also by large bodies of several tens of meters in
diameter. Therefore, small extinct comets might be searched for along
the orbits of meteoroid streams during periods of meteor shower
activity. This inference is confirmed by the detection of 17 objects
of some meters to some tens of meters, which passed within a few
million km of the Earth. They were observed by Barabanov et al. (2001)
during the period of activity of the Capricornids, Perseids, Leonids,
and Coma Berenicids meteor showers, near the radiant positions of
these showers, using 60-cm and 1-m telescopes with CCD-cameras ST-6,
at the Zvenigorod (Moscow district) and Simeiz (Crimea)
observatories of the Institute of Astronomy, Russian Academy of Sciences.
Copyright ESO 2003