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Domain and Website Information:
etno.de
About site:
Domain name - etno.de
Site title - etno.de - This website is for sale! - etno Resources and Information.
Go to website - etno.de - This website is for sale! - etno Resources and Information.
Words count at etno.de:
etno - 6
this - 4
you - 4
domain - 4
sale - 3
the - 3
sedo - 3
website - 2
and - 2
See complete list
Site GEO location
Location Country - Germany
Provider - SEDO GmbH
Site Logo
There is no Open Graph data at etno.de
Information for domain etno.de
IP address:
Domain name servers:
ns2.sedoparking.com ns1.sedoparking.com
All records:
☆ etno.de. 21600 IN NS ns1.sedoparking.com.
☆ etno.de. 21600 IN NS ns2.sedoparking.com.
☆ etno.de. 3600 IN MX 0 localhost.
☆ etno.de. 3600 IN TXT "v=spf1 -all"
☆ etno.de. 300 IN A 64.190.63.222
☆ etno.de. 21600 IN SOA ns1.sedoparking.com. hostmaster.sedo.de. 2018051601 86400 10800 604800 86400
Whois server information for etno.de
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Domain: etno.de
Nserver: ns1.sedoparking.com
Nserver: ns2.sedoparking.com
Status: connect
Changed: 2016-03-29T23:43:32+02:00
Brief facts about etno:
A trans-Neptunian object, also written transneptunian object, is any minor planet in the Solar System that orbits the Sun at a greater average distance than Neptune, which has an orbital semi-major axis of 30.1 astronomical units. Typically, TNOs are further divided into the classical and resonant objects of the Kuiper belt, the scattered disc and detached objects with the sednoids being the most distant ones. As of October 2020, the catalog of minor planets contains 678 numbered and more than 2,000 unnumbered TNOs. The first trans-Neptunian object to be discovered was Pluto in 1930. It took until 1992 to discover a second trans-Neptunian object orbiting the Sun directly, 15760 Albion. The most massive TNO known is Eris, followed by Pluto, Haumea, Makemake, and Gonggong. More than 80 satellites have been discovered in orbit of trans-Neptunian objects. TNOs vary in color and are either grey-blue or very red.
Dwarf planet - A dwarf planet is a small planetary-mass object that is in direct orbit around the Sun, massive enough to be gravitationally rounded, but insufficient to achieve orbital dominance like the eight classical planets of the Solar System.
Mesoplanet - Mesoplanets are planetary-mass objects with sizes smaller than Mercury but larger than Ceres. The term was coined by Isaac Asimov. Assuming size is defined in relation to equatorial radius, mesoplanets should be approximately 500 km to 2,500 km in radius.
Nemesis (hypothetical star) - Nemesis was a hypothetical red dwarf or brown dwarf, originally postulated in 1984 to be orbiting the Sun at a distance of about 95,000 AU, somewhat beyond the Oort cloud, to explain a perceived cycle of mass extinctions in the geological record, which seem to occur more often at intervals of 26...
Planet Nine - Planet Nine is a hypothetical ninth planet in the outer region of the Solar System.
Sednoid - A sednoid is a trans-Neptunian object with a large semi-major axis and a high perihelion, similar to the orbit of Sedna. The consensus among astronomers is that there are only three objects that are known from this population: 90377 Sedna, 2012 VP113, and 541132 Leleākūhonua.
Small Solar System body - A small Solar System body is an object in the Solar System that is neither a planet, a dwarf planet, nor a natural satellite.
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