JPEG (97K)
Time: March 25, 1996, 17h40m GMT
Camera: 55mm F1.8 lens, Fuji HG1600 film, 40 sec exposure
Location: Kameoka City, Kyoto Pref.
by T. Fujiwara
The comet discovered by Yuji Hyakutake () in Hayato-machi, Kagoshima, Japan, on January 31 (JST) might become a great comet in March and April this year.
The comet is traveling toward the sun due at perihelion of 0.23AU from the sun on May 1. On its way to the sun the comet comes near Earth in late March. The closest approach takes place on March 25, and the distance is only 0.10AU (about 40 times of the distance to the moon). Because the comet passes near Earth, it moves very rapidly in the sky from Bootes to Perseus in late March (see the figures below).
The magnitude around March 25 is expected to be 0mag or so,
bright enough for the naked eye.
However, one might not feel as bright as usual stars,
since the comet should be diffuse and extended.
The tail will be faint, because a prominent dust tail usually develops
after approaching the sun.
I recommend viewing the comet with binoculars.
* (Comment added on March 24) The comet is bright! The tail is faint but very long!
I would like to recommend viewing with the naked eye as well.
In April the comet approaches the sun and a dust tail will develop. In late April, the comet gets close to the sun and it will soon sets in the evening sky. In May, unfortunately, the comet goes to the south side of the solar system, so that it cannot be observed from the Northern Hemisphere. (February 29)
Finder chart for late March
(positions at 21h JST=12h GMT /
21h GMT /
21h PST=24+5h GMT)
Finder chart for April
(positions at 20h JST=11h GMT /
21h GMT /
20h PST=24+4h GMT)
Visibility Chart
(for locations 135°E, 35°N /
0°, 50°N /
120°W, 35°N)
These charts were created with StellaNavigator (ASCII/AstroArts).