Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q3303> ?p ?o }
- Q3303 subject Q7152472.
- Q3303 subject Q8266666.
- Q3303 subject Q8412960.
- Q3303 abstract "Enceladus (pronounced /ɛnˈsɛlədəs/) is the sixth-largest moon of Saturn. It is 500 kilometers (310 mi) in diameter, about a tenth of that of Saturn's largest moon, Titan. Enceladus is mostly covered by fresh, clean ice, reflecting almost all the sunlight that strikes it, making its surface temperature at noon reach only −198 °C (−324.4 °F). Despite its small size, Enceladus has a wide range of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrains that formed as recently as 100 million years ago.Enceladus was discovered in 1789 by William Herschel, but little was known about it until the two Voyager spacecraft passed nearby in the early 1980s. In 2005, the Cassini spacecraft started multiple close flybys of Enceladus, revealing its surface and environment in greater detail. In particular, Cassini discovered water-rich plumes venting from the south polar region. Cryovolcanoes near the south pole shoot geyser-like jets of water vapor, other volatiles, and solid material, including sodium chloride crystals and ice particles, into space, totaling approximately 200 kilograms (440 lb) per second. Over 100 geysers have been identified. Some of the water vapor falls back as "snow"; the rest escapes, and supplies most of the material making up Saturn's E ring. According to NASA scientists, the plumes are similar in composition to comets. In 2014, NASA reported that Cassini found evidence for a large south polar subsurface ocean of liquid water with a thickness of around 10 km (6.2 mi).These geyser observations, along with the finding of escaping internal heat and very few (if any) impact craters in the south polar region, show that Enceladus is geologically active today. Enceladus is, like many satellites in the extensive systems of the giant planets, trapped in an orbital resonance. Its resonance with Dione excites its orbital eccentricity, which is damped by tidal forces, tidally heating its interior, and possibly driving the geological activity.".
- Q3303 albedo "0.99".
- Q3303 apparentMagnitude "11.7".
- Q3303 discovered "1789-08-28".
- Q3303 discoverer Q14277.
- Q3303 escapeVelocity "860.4".
- Q3303 formerName "Saturn II".
- Q3303 maximumTemperature "145.0".
- Q3303 maximumTemperature "145.15".
- Q3303 meanTemperature "75.0".
- Q3303 meanTemperature "75.15".
- Q3303 minimumTemperature "32.9".
- Q3303 minimumTemperature "33.15".
- Q3303 thumbnail PIA17202_-_Approaching_Enceladus.jpg?width=300.
- Q3303 wikiPageExternalLink planetarynames.wr.usgs.gov.
- Q3303 wikiPageExternalLink search.php?x=20&y=7&search=Enceladus.
- Q3303 wikiPageExternalLink PIA19060_JPL-20150313-pCassin-0001-640.mp4.
- Q3303 wikiPageExternalLink Enceladus.
- Q3303 wikiPageExternalLink target.
- Q3303 wikiPageExternalLink enceladus_comp.pdf.
- Q3303 wikiPageExternalLink moonDetails.cfm?pageID=5.
- Q3303 wikiPageExternalLink MultimediaProductsCharm.
- Q3303 wikiPageExternalLink solarsystem.nasa.gov.
- Q3303 wikiPageExternalLink profile.cfm?Object=Sat_Enceladus.
- Q3303 wikiPageExternalLink Enceladus.mov.
- Q3303 wikiPageExternalLink turn-of-enceladus.html.
- Q3303 wikiPageExternalLink Enceladus_OLEB_online_published_paper.pdf.
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- Q3303 wikiPageExternalLink enceladus.htm.
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