The duration of this shower extends from January 15 to 30. At maximum on
January 20, meteors can be expected to reach an hourly rate of 2-5 from a
radiant of RA=140 deg, DECL=-9 deg.
The first apparent observation of this shower was made by Ronald A. McIntosh
on January 15, 1929. Four plotted meteors revealed a radiant of RA=132.2 deg,
DECL=-7.0 deg. The shower does not appear in any records prior to the 20th
century, nor in the major radiant catalogs of Ernst Ípik (1934) and Cuno
Hoffmeister (1948). McIntosh's observation remained the only detection of this
shower by Southern Hemisphere observers up to 1935, so that it was not included
in his "An Index to Southern Meteor Showers," which appeared in the Monthly
Notices of the Royal Astronomical Society in that year.
The first determination of this shower's hourly rate was made during January
20/21 and 24/25, 1971, by three members of the American Meteor Society. Karl
Simmons (Florida), John West (Texas) and T. Recascino (New Jersey) detected
maximum rates of 2-3 during this period when the limiting magnitude was 5.5-6.0.
Perhaps the greatest knowledge of this meteor shower has come from the
observations of the Western Australia Meteor Section (WAMS) made during the
period of 1979 to 1986. During that first year, observers detected Alpha Hydrids
during January 20-30, and determined the date of maximum as January 25. The
average radiant was RA=140 deg, DECL=-9 deg, while the maximum ZHR was given as
8.51+/-1.84. Other details uncovered included an average magnitude of 3.15
(based on 54 meteors) and the fact that 10.2% of the meteors left trains. The
meteors also tended to display three colors: 56.2% were white, 37.5% were yellow
and 6.3% were blue. During 1980, Alpha Hydrids were detected during January
12-27, with a maximum ZHR of 1.90+/-0.19 occurring on January 16 from RA=136
deg, DECL=-10 deg. The hourly rates indicated possible irregular activity coming
from this radiant. Observations in the following years revealed this to be true,
with hourly rates barely attaining 2 per hour during 1982, 1984 and 1986, while
rates reached 4-5 in 1983 and 3-4 in 1985.
Members of the WAMS succeeded in determining a series of radiant positions
during 1980, which display a definite eastward movement. Using only those days
for which 2 or more positions could be averaged, the Author determined four
positions: RA=133 deg, DECL=-10 deg on January 16/17, RA=138.8 deg, DECL=-10.3
deg on January 18/19, RA=141 deg, DECL=-9 deg on January 22/23, and RA=146 deg,
DECL=-10 deg on January 26/27.
The Author has sought to determine the orbit of this stream and has
succeeded in finding 2 photographic members (one in MP1961 and one in CF1973)
and 19 radio members (M1986). Two apparent streams were revealed. The first
radiant is composed of 4 radio meteors and the 2 photographic meteors and is
apparently responsible for the visual activity. The duration is January 10-28.
The nodal passage comes on January 17, with the radiant then being at RA=135.9
deg, DECL=-10.0 deg. The radiant's daily motion is +0.98 deg in RA and -0.57 deg
in DECL. The other stream is made up of 15 radio meteors and is active during
January 11-30. The nodal passage occurs on January 21 from RA=149.0 deg,
DECL=-9.1 deg. The daily motion is +0.88 deg in RA and -0.51 deg in DECL. It is
possible that, since the radar data never adequately covered the period of
January 20-25, the maximums of both streams may occur later than the indicated
dates of the nodal passages.