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Domain and Website Information:
hale-bopp.it
About site:
Domain name - hale-bopp.it
Site title - WordPress – WordPress Description
Go to website - WordPress – WordPress Description
Words count at hale-bopp.it:
hale - 2
bopp - 2
info - 2
description - 1
format - 1
radio - 1
organizzazione - 1
meeting - 1
convegni - 1
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Site GEO location
Location Country - Italy
City/Town - Arezzo
Provider - Aruba S.p.A.
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Information for domain hale-bopp.it
IP address:
Domain name servers:
dns4.arubadns.cz dns2.technorail.com dns3.arubadns.net dns.technorail.com
All records:
☆ hale-bopp.it. 3600 IN A 31.11.36.37
☆ hale-bopp.it. 3600 IN TXT "v=spf1 include:_spf.aruba.it ~all"
☆ hale-bopp.it. 3600 IN MX 10 mx.hale-bopp.it.
☆ hale-bopp.it. 3600 IN NS dns2.technorail.com.
☆ hale-bopp.it. 3600 IN NS dns.technorail.com.
☆ hale-bopp.it. 3600 IN NS dns3.arubadns.net.
☆ hale-bopp.it. 3600 IN NS dns4.arubadns.cz.
☆ hale-bopp.it. 3600 IN SOA dns.technorail.com. hostmaster.hale-bopp.it. 1 86400 7200 2592000 3600
Whois server information for hale-bopp.it
Brief facts about hale bopp:
Comet Hale–Bopp is a comet that was one of the most widely observed of the 20th century and one of the brightest seen for many decades. Alan Hale and Thomas Bopp discovered Comet Hale–Bopp separately on July 23, 1995, before it became visible to the naked eye. It is difficult to predict the maximum brightness of new comets with any degree of certainty, but Hale–Bopp exceeded most predictions when it passed perihelion on April 1, 1997, reaching about magnitude −1.8. It was visible to the naked eye for a record 18 months, due to its massive nucleus size. This is twice as long as the Great Comet of 1811, the previous record holder. Accordingly, Hale–Bopp was dubbed the great comet of 1997.
Comet Hyakutake - Comet Hyakutake is a comet discovered on 31 January 1996. It was dubbed the Great Comet of 1996; its passage to within 0.1 AU of the Earth on 25 March was one of the closest cometary approaches of the previous 200 years.
Lists of comets - Non-periodic comets are seen only once. They are usually on near-parabolic orbits that will not return to the vicinity of the Sun for thousands of years, if ever. Periodic comets usually have elongated elliptical orbits, and usually return to the vicinity of the Sun after a number of decades.
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