Where is Hale-Bopp now? The Great Comet of 1997 [
http://www.jpl.nasa
], one of the largest and most active comets ever, is outbound [
http://antwrp.gsfc.
] about 400 million miles from the sun. Too faint for viewing without telescopes or binoculars, Hale-Bopp is presently positioned in the very southerly constellation of Pictor. This "negative" image [
http://www.eso.org/
] (black stars against white sky) of Hale-Bopp is the result of a 1 hour time exposure using the 1-metre European Southern Observatory [
http://search.eso.o
] Schmidt telescope on January 5. Clearly the comet still has a substantial tail [
http://antwrp.gsfc.
], blown by the solar wind [
http://antwrp.gsfc.
], that points generally away from the sunward direction. But look closely. A spiky "anti-tail" is also visible [
http://cfa-www.harv
] pointing toward the sun! It is likely that this anti-tail is composed of dust grains released from the comet nucleus [
http://antwrp.gsfc.
] which are too large to be easily pushed by the solar wind. As Hale-Bopp recedes [
http://www.pha.jhu.
] from the sun its activity will subside but astronomers are still uncertain as to how long its tails will last. After a swing through the outer solar system and the Oort cloud [
http://www.windows.
], Hale-Bopp will pass through the inner solar system again ... around the year 5400.
Explanation
Where is Hale-Bopp now? The Great Comet of 1997 [
http://www.jpl.nasa
], one of the largest and most active comets ever, is outbound [
http://antwrp.gsfc.
] about 400 million miles from the sun. Too faint for viewing without telescopes or binoculars, Hale-Bopp is presently positioned in the very southerly constellation of Pictor. This "negative" image [
http://www.eso.org/
] (black stars against white sky) of Hale-Bopp is the result of a 1 hour time exposure using the 1-metre European Southern Observatory [
http://search.eso.o
] Schmidt telescope on January 5. Clearly the comet still has a substantial tail [
http://antwrp.gsfc.
], blown by the solar wind [
http://antwrp.gsfc.
], that points generally away from the sunward direction. But look closely. A spiky "anti-tail" is also visible [
http://cfa-www.harv
] pointing toward the sun! It is likely that this anti-tail is composed of dust grains released from the comet nucleus [
http://antwrp.gsfc.
] which are too large to be easily pushed by the solar wind. As Hale-Bopp recedes [
http://www.pha.jhu.
] from the sun its activity will subside but astronomers are still uncertain as to how long its tails will last. After a swing through the outer solar system and the Oort cloud [
http://www.windows.
], Hale-Bopp will pass through the inner solar system again ... around the year 5400.
Explanation