Throughout the first week of April, the comet is making a wonderfully photogenic pass by the Andromeda Galaxy, M31, presenting astrophotographers at northerly locations with a unique opportunity. The image above was taken on the morning of April 4th, and this deep image was taken on March 30th. The comet passed closest to the showpiece galaxy in the early hours of April 4th UT. The tail continues to widen as seen from Earth's perspective.
The comet is now actually higher before dawn, in the northeastern sky. But the waning Moon is up then (though dimmer every morning; last quarter was on the 3rd). Evening is when northern imagers can catch this departing visitor with no interference from either twilight or moonlight. The farther north of 40° latitude you are the better.
Some recent brightness estimates put the comet at about 4th magnitude, slightly fainter than M31. Other observers say it's slightly brighter than the galaxy. This depends on the darkness and quality of your sky; the comet's head is more concentrated and has a higher surface brightness than the galaxy's inner portion.
As for visual sightings, from my latitude of 43° I could not see it naked-eye on March 30th, though it was still easily visible in my 70mm spotting scope.
From latitude 49° Alan Whitman in Penticton, British Columbia,writes,
"On March 31st with excellent transparency, Comet PanSTARRS was visible with the unaided eye exactly two hours after sunset. It is now in the same binocular field of view as 3.4-magnitude M31, and the comet is about 0.5 magnitude brighter than the galaxy, making the comet about magnitude 3.
"In a 4.2-inch Astroscan at 64x, the broad, fanned tail was about 0.7° long, sharper and slightly curved on the preceeding edge. The pseudonucleus is nearly stellar."
Send us your observations and photographs! Post your pix in the Comet PanSTARRS section of our Photo Gallery.
Also, this amazing shot was taken by Michael Jaeger and Hohe Tauern on April 1st.