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Comet Hale-Bopp in the Outer
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| Title |
Comet Hale-Bopp in the Outer Solar System |
| Explanation |
Whatever became of Comet Hale-Bopp [ http://antwrp.gsfc.nasa.gov/apod/ap010326.html http://apod.gsfc.nasa.gov/cgi-bin/apod/apod_search?Comet+Hale-Bopp ]? The brightest comet [ http://www.nineplanets.org/comets.html ] in recent years has continued into the outer Solar System [ http://www.exploratorium.edu/ronh/solar_system/ ] and is now farther from the Sun [ http://www.nineplanets.org/sol.html ] than Saturn [ http://www.solarviews.com/eng/saturn.htm ]. To the surprise of many, Comet Hale-Bopp [ http://www.jpl.nasa.gov/comet/ ] is still active, continuing to spew gas, ice and dust particles out into space. Pictured above earlier this month, Comet Hale-Bopp [ http://antwrp.gsfc.nasa.gov/apod/hale_bopp.html ] can be seen in the Southern Hemisphere [ http://antwrp.gsfc.nasa.gov/apod/ap001223.html ] with a moderate sized-telescope. The continued activity of Comet Hale-Bopp [ http://antwrp.gsfc.nasa.gov/apod/ap001227.html ] may be due to the large size of its nucleus [ http://antwrp.gsfc.nasa.gov/apod/ap000805.html ] - estimated to be about 50 kilometers across. The unusual dotted appearance [ http://www.eso.org/outreach/press-rel/pr-2001/phot-07-01.html#techinfo ] of most stars in the above image [ http://www.eso.org/outreach/press-rel/pr-2001/phot-07-01.html ] is due to the 14 discrete exposures that were centered on the comet and not the stars. |
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Announcing Comet Hale-Bopp
| Title |
Announcing Comet Hale-Bopp |
| Explanation |
The pictured fuzzy patch may become one of the most spectacular comets this century. Although it is very hard to predict how bright a comet [ http://seds.lpl.arizona.edu/billa/tnp/comets.html ] will become, Comet Hale-Bopp [ http://encke.jpl.nasa.gov/hale_bopp_info.html ], named for its discoverers [ http://encke.jpl.nasa.gov/hale_bopp/discoverers.html ], was spotted farther from the Sun [ http://antwrp.gsfc.nasa.gov/apod/ap950813.html ] than any previous comet - a good sign that it could become very bright, easily visible to the naked eye. This picture was taken on July 25th 1995, only two days after its discovery. A comet [ http://www.c3.lanl.gov/~cjhamil/SolarSystem/comet.html ] bright enough to see without a telescope occurs only about once a decade. The large coma [ http://antwrp.gsfc.nasa.gov/apod/lib/glossary.html#coma ] and long tail [ http://antwrp.gsfc.nasa.gov/apod/lib/glossary.html#comet ] of bright comets are so unusual and impressive that they have been considered omens of change by many cultures. A comet does not streak by in few seconds - but it may change its position and structure noticeably from night to night. Tomorrow's picture: An Orbiting Iceberg |
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Comet Hale-Bopp Update
| Title |
Comet Hale-Bopp Update |
| Explanation |
Will comet Hale-Bopp [ http://www.halebopp.com/ ] become the brightest comet of the Century in early 1997? Since its discovery in July [ http://antwrp.gsfc.nasa.gov/apod/ap950820.html ] this year, Hale-Bopp [ http://encke.jpl.nasa.gov/hale_bopp_info.html ] has caused much speculation. Even though it is still beyond the orbit of Jupiter it is astonishingly bright and expected to get much brighter as it plunges inward, toward the Sun. In this latest Hubble Space Telescope image [ http://www.stsci.edu/pubinfo/PR/95/41.html ] a bright clump of material (above center) has apparently been ejected by evaporation and the rotation of the icy nucleus [ http://antwrp.gsfc.nasa.gov/apod/lib/glossary.html#comet ] (below center). Astronomers are using this and other observations to try to figure out if Hale-Bopp is really a giant comet or a smaller object which will fizzle out sooner than expected as it approaches the Sun. |
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Comet Hale-Bopp Fades
| Title |
Comet Hale-Bopp Fades |
| Explanation |
Comet Hale-Bopp has faded in the past few weeks. For Hale-Bopp [ http://newproducts.jpl.nasa.gov/comet/ ], promised as the Great Comet of 1997, this was a bit of a disappointment -- but not entirely unexpected. Comet Hale-Bopp [ http://antwrp.gsfc.nasa.gov/apod/ap960729.html ] continues to approach the Sun [ http://antwrp.gsfc.nasa.gov/apod/ap960916.html ] - making the comet itself brighten, but now the Earth [ http://antwrp.gsfc.nasa.gov/apod/ap960819.html ] is moving away from it - making the comet appear to dim. Experts disagree on just how bright Hale-Bopp [ http://encke.jpl.nasa.gov/hale_bopp_info.html ] will become. Optimists hope it will eventually outshine Comet Hyakutake [ http://antwrp.gsfc.nasa.gov/apod/lib/hyakutake.html ], but some pessimists now expect no better than 3rd magnitude - hardly visible from well-lit cities [ http://antwrp.gsfc.nasa.gov/apod/ap960617.html ]. Comet Hale-Bopp [ http://www.eso.org/comet-hale-bopp/ ] still appears to be, however, a very large comet, and is sure to show much activity as it nears the Sun. The comet should reach peak brightness in March 1997. [ http://newproducts.jpl.nasa.gov/comets/ephemjpl3.html ] This image [ http://www.eso.org/comet-hale-bopp/comet-hale-bopp-summary-sep13-96-rw.html ] was taken on August 18th and shows gas shed from the nucleus of the comet. |
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The Dust and Ion Tails of Co
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| Title |
The Dust and Ion Tails of Comet Hale-Bopp |
| Explanation |
In 1997, Comet Hale-Bopp [ http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_ts?Bopp ]'s "intrinsic" brightness exceeded any comet since 1811 [ http://cometography.com/lcomets/1811f1.html ]. Since it peaked on the other side of the Earth's orbit, however, the comet "appeared" only brighter than any comet in two decades [ http://cometography.com/lcomets/1975v1.html ]. Visible above are the two tails [ http://antwrp.gsfc.nasa.gov/apod/ap960502.html ] shed by Comet Hale-Bopp [ http://www.jpl.nasa.gov/comet/ ]. The blue ion tail [ http://www-spof.gsfc.nasa.gov/istp/events/halebopp/disconnect/ ] is composed of ionized [ http://csep10.phys.utk.edu/astr162/lect/light/ionization.html ] gas molecules, of which carbon monoxide [ http://www.cpsc.gov/cpscpub/pubs/466.html ] particularly glows blue when reacquiring electrons [ http://www-spof.gsfc.nasa.gov/Education/welect.html ]. This tail [ http://antwrp.gsfc.nasa.gov/htmltest/gifcity/comet.html ] is created by the particles from the fast solar wind [ http://antwrp.gsfc.nasa.gov/apod/ap000318.html ] interacting with gas from the comet's head. The blue ion tail [ http://antwrp.gsfc.nasa.gov/apod/ap970514.html ] points directly away from the Sun [ http://www.seds.org/nineplanets/nineplanets/sol.html ]. The light colored dust tail [ http://antwrp.gsfc.nasa.gov/apod/ap970403.html ] is created by bits of grit that have come off the comet's nucleus [ http://antwrp.gsfc.nasa.gov/apod/ap000805.html ] and are being pushed away by the pressure of light [ http://antwrp.gsfc.nasa.gov/apod/ap000526.html ] from the Sun. This tail points "nearly" away from the Sun. The above photograph [ http://www.celestialimage.com/page101.html ] was taken in March 1997. |
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Comet Hale-Bopp Over the Sup
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| Title |
Comet Hale-Bopp Over the Superstition Mountains |
| Explanation |
Four years ago, Comet Hale-Bopp [ http://galileo.ivv.nasa.gov/comet/ ] was discovered [ http://antwrp.gsfc.nasa.gov/apod/ap950820.html ] out near Jupiter [ http://www.seds.org/nineplanets/nineplanets/jupiter.html ] falling toward the inner Solar System [ http://spacelink.nasa.gov/Instructional.Materials/Curriculum.Support/Space.Science/Our.Solar.System/.index.html ]. Two years ago, it provided spectacular pictures [ http://antwrp.gsfc.nasa.gov/cgi-bin/cossc/apod_search?Hale-Bopp ] as it neared its closest approach to the Sun [ http://shutter.vet.ohio-state.edu/astronomy/faq/index.htm ]. Still today, spectacular pictures [ http://antwrp.gsfc.nasa.gov/apod/ap970723.html ] of the brightest comet of the 1990s are surfacing. Above, Comet Hale-Bopp was photographed in 1997 behind the Superstition Mountains [ http://www.goodnet.com/~rfidler/Page/Superstitions.htm ] in Arizona [ http://www.state.az.us/ ]. Clearly visible are the comets white dust tail [ http://antwrp.gsfc.nasa.gov/apod/ap960326.html ] that shines by reflected sunlight, and the blue ion tail [ http://antwrp.gsfc.nasa.gov/apod/ap970514.html ] that shines by glowing gas. Currently, there are several comets visible [ http://comets.amsmeteors.org/comets/current_comets.html ] from the proper location with a small telescope. A comet visible to the unaided eye [ http://encke.jpl.nasa.gov/bright_comet.html ] appears about once every five years. |
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