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149.62.185.42


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ns1.host-anycast.it ns2.host-anycast.com


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☆ plutino.it. 354 IN A 149.62.185.42
☆ plutino.it. 354 IN MX 10 mailgw01.host.it.
☆ plutino.it. 354 IN MX 10 mailgw02.host.it.
☆ plutino.it. 21600 IN NS ns2.host-anycast.com.
☆ plutino.it. 21600 IN NS ns1.host-anycast.it.
☆ plutino.it. 3594 IN TXT "v=spf1 mx a include:spf.host.it -all"
☆ plutino.it. 3594 IN SOA ns1.host-anycast.it. dns.host.it. 2023033101 10800 3600 1209600 3600


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Brief facts about plutino:

In astronomy, the plutinos are a dynamical group of trans-Neptunian objects that orbit in 2:3 mean-motion resonance with Neptune. This means that for every two orbits a plutino makes, Neptune orbits three times. The dwarf planet Pluto is the largest member as well as the namesake of this group. The next largest members are Orcus, 2003 AZ84, and Ixion. Plutinos are named after mythological creatures associated with the underworld. Plutinos form the inner part of the Kuiper belt and represent about a quarter of the known Kuiper belt objects. They are also the most populous known class of resonant trans-Neptunian objects. The first plutino after Pluto itself, 1993 RO, was discovered on September 16, 1993.

Resonant Trans-Neptunian Object - In astronomy, a resonant trans-Neptunian object is a trans-Neptunian object in mean-motion orbital resonance with Neptune. The orbital periods of the resonant objects are in a simple integer relations with the period of Neptune, e.g. 1:2, 2:3, etc.

Plutinos

 

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