cahya/wikipedia-simple-en huggingface dataset:
Vung Tau

Vung Tau (Vietnamese: Vũng Tàu) is a city in Ba Ria-Vung Tau Province, Vietnam. This city has a population of 240,000 and an area of 154.0 km2. This is a petroleum and tourism centre of Vietnam.

History 
Vung Tau is located about 120 km northeast of Ho Chi Minh City. Vung Tau town was founded by French colonists under the administration of Paul Doumer, then the Governor General of French Indochina. This city borders Vietnam Sea and has several beautiful beaches.

Cities in Vietnam
Media Access Control

A Media Access Control address (often shortened to MAC address) is a 48-bit code which allows a computer to be part of a computer network.  Usually, a computer has only one MAC address.  Each computer has a MAC address which identifies it uniquely on the network.  No other device on the Internet will have the same MAC address. A MAC address contains two pairs of 24-bit hexadecimals: the first pair is the international standard identifier of the International Organization for Standardization (ISO) and the last pair is the serial number for the network interface card to uniquely identify the card.

Computer networking
Arabic Wikipedia

The Arabic Wikipedia () is the Arabic language version of Wikipedia. It started in September 2001.

It was the 23rd largest edition of Wikipedia by article count, but grew to 17th largest edition.

As of August 2014, it has over 300,000 articles, over 1,350,000 pages, over 625,000 registered users and over 15,000 files.

It has been blocked in Syria.

References

Other websites
Arabic Wikipedia's main page

Wikipedias
Websites established in 2001
French Wikipedia

The French Wikipedia, the free Wikipedia ( or ) is the French language edition of Wikipedia, spelled Wikipédia. It started in March 2001.  It is the largest Wikipedia in a Romance language.  It was the third largest Wikipedia after the English language and German language editions, but dropped to sixth.

As of  , it has about  articles.

References

Other websites 

 French Wikipedia, the Free Wikipedia's Main page7

Wikipedias
Websites established in 2001
German Wikipedia

The German Wikipedia () is the German language edition of Wikipedia. Founded 16 March 2001, it is the second-oldest and the first non-English-language Wikipedia.

By count of articles, it is the third largest Wikipedia, after the English Wikipedia and the Swedish Wikipedia. As of  , it has about  articles.

References

Other websites 

 German Wikipedia's Main page 

Wikipedias
Websites established in 2001
Mundilfari (moon)

Mundilfari or Saturn XXV, is a moon of Saturn. It was found by Brett J. Gladman, et al. in 2000, and given the designation S/2000 S 9.

Mundilfari is about 5.6 kilometres in diameter, and orbits Saturn at an average distance of 18,360,000 km in 928.806 days, at an inclination of 170° to the ecliptic (150° to Saturn's equator), with an eccentricity of 0.198.

Mundilfari may have formed from debris knocked off of Phoebe by big impacts at some point in the solar system's history.

It was named in August 2003 from Norse mythology, where Mundilfari is a Jotun or giant who is the father of the goddess Sol and the god Mani.

References
 IAUC 7538: S/2000 S 7, S/2000 S 8, S/2000 S 9 2000 December 7 (discovery)
 MPEC 2000-Y15: S/2000 S 1, S/2000 S 2, S/2000 S 7, S/2000 S 8, S/2000 S 9 2000 December 19 (discovery and ephemeris)
 IAUC 8177: Satellites of Jupiter, Saturn, Uranus 2003 August 8 (naming the moon)

Saturn's moons
S/2006 S 1

S/2006 S 1 is an unnamed moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on June 26, 2006, from observations taken between January 4 and April 30, 2006.

S/2006 S 1 is about 6 kilometres in diameter, and orbits Saturn at an average distance of 18,930,200 km in 972.407 days, at an inclination of 154.2° to the ecliptic (175.4° to Saturn's equator), with an eccentricity of 0.1303.

References 
 Institute for Astronomy Saturn Satellite Data
 IAUC 8727: Satellites of Saturn 2006 June 30 (discovery)
 MPEC 2006-M45: Eight New Satellites of Saturn 2006 June 26 (discovery and ephemeris)

Saturn's moons
S/2004 S 17

S/2004 S 17 is an unnamed moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 13, 2004, and March 5, 2005.

S/2004 S 17 is about 4 kilometres in diameter, and orbits Saturn at an average distance of 19,099,000 km in 985.453 days, at an inclination of 167° to the ecliptic (162° to Saturn's equator), with an eccentricity of 0.226.

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn 2005 May 4 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn 2005 May 3 (discovery and ephemeris)

Saturn's moons
Bergelmir (moon)

Bergelmir or Saturn XXXVIII (provisional designation S/2004 S 15) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 9, 2005.

Bergelmir is about 6 kilometres in diameter, and orbits Saturn at an average distance of 19,372,000 km in 1006.659 days, at an inclination of 157° to the ecliptic (134° to Saturn's equator), with an eccentricity of 0.152.

It was named in April 2007 after Bergelmir, a giant from Norse mythology and the grandson of Ymir, the primordial giant. Bergelmir and his wife alone among their kind were the only survivors of the enormous deluge of blood from Ymir's wounds when he was killed by Odin and his brothers at the dawn of time. Bergelmir then became the progenitor of a new race of giants.

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn May 4, 2005 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn May 3, 2005 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (naming the moon)

Saturn's moons
Narvi (moon)

Narvi ( ) or Saturn XXXI is a moon of Saturn. It was discovered by a team of astronomers led by Scott S. Sheppard in 2003, and given the designation S/2003 S 1.

Description 
Narvi is about 7 kilometres in diameter, and orbits Saturn at an average distance of 19,371,000 km in 1006.541 days, at an inclination of 137° to the ecliptic (109° to Saturn's equator), with an eccentricity of 0.320.

Naming 
It was named in January 2005 after Narvi from Norse mythology, also known as Narfi or Nari, a son of Loki by Sigyn who was killed to punish Loki for his crimes. The gods turned his brother Váli into a slavering wolf who tore his throat out. His entrails were used to bind Loki to a stone slab for all eternity, or at least until Ragnarok. The name was approved by the IAU Working Group on Planetary System Nomenclature on January 21, 2005.

Other websites 
 IAU Working Group for Planetary System Nomenclature
 IAUC 8116: Satellites of Jupiter and Saturn 2003 April 11 (discovery)
 MPEC 2003-G39: S/2003 S 1 2003 April 8 (discovery and ephemeris)
 IAUC 8471: Satellites of Saturn 2005 January 21 (naming the moon)

Saturn's moons
Suttungr (moon)

Suttungr or Saturn XXIII, is a moon of Saturn. It was found by Brett J. Gladman, et al. in 2000, and given the designation S/2000 S 12.

Suttungr is about 5.6 kilometres in diameter, and orbits Saturn at an average distance of 19,667,000 km in 1029.703 days, at an inclination of 174° to the ecliptic (151° to Saturn's equator), with an eccentricity of 0.131.

Suttungr may have formed from debris knocked off of Phoebe at some point in the past.

It was named in August 2003 from Norse mythology, where Suttung is a Jotun or giant who once owned the mead of poetry.

The name was said as Suttung in IAU Circular 8177. However, the IAU Working Group on Planetary System Nomenclature later decided to add the nominative case ending -r to the base form Suttung.

References 
 IAUC 7548: S/2000 S 12 2000 December 23 (discovery)
 MPEC 2000-Y33: S/2000 S 12 2000 December 22 (recovery/discovery and ephemeris)
 IAUC 8177: Satellites of Jupiter, Saturn, Uranus 2003 August 8 (naming the moon Suttung)
 IAUC 8471: Satellites of Saturn 2005 January 21 (correcting the name)

Saturn's moons
Hati (moon)

Hati or Saturn XLIII (provisional designation S/2004 S 14) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 11, 2005.

Hati is about 6 kilometers in diameter, and orbits Saturn at an average distance of 20,303,000 km in 1080.099 days, at an inclination of 163° to the ecliptic (165° to Saturn's equator), with an eccentricity of 0.291.

It was named in April 2007 after Hati, a giant wolf from Norse mythology, son of Fenrisulfr and twin brother of Skoll.

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn 2005 May 4 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn 2005 May 3 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (naming the moon)

Saturn's moons
S/2004 S 12

S/2004 S 12 is an unnamed moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 9, 2005.

S/2004 S 12 is about 5 kilometres in diameter, and orbits Saturn at an average distance of 19,906,000 km in 1048.541 days, at an inclination of 164° to the ecliptic (162° to Saturn's equator), with an eccentricity of 0.396.

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn 2005 May 4 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn 2005 May 3 (discovery and ephemeris)

Saturn's moons
Farbauti (moon)

Farbauti or Saturn XL (also called S/2004 S 9) is a moon of Saturn. It was found by Scott S. Sheppard, David C. Jewitt, and Jan Kleyna on December 12, 2004. Farbauti was found using the Mauna Kea Observatory and is the 40th moon from Saturns surface. The public did not know about Farbauti until May 4, 2005.

Farbauti is 5 kilometres wide, and 20,291,000 kilometres from Saturns surface. Farbauti travels around Saturn (orbit) once every 1079 days.

The moon was named in April 2007 after the "storm giant" Fárbauti, father of Loki in Norse mythology.

Other websites 
 David C.Jewitt's New Satellites of Saturn page
 The American Government listing of moons of the Solar System
 Harvard University notes

Saturn's moons
Thrymr (moon)

Thrymr or Saturn XXX, is a moon of Saturn. It was found by Gladman, et al. in 2000, and given the designation S/2000 S 7.

Thrymr is about 5.6 kilometres in diameter, and orbits Saturn at an average distance of 20,810,000 km in 1120.809 days, at an inclination of 175° to the ecliptic (151° to Saturn's equator), with an eccentricity of 0.453.

Thrymr may have formed from debris knocked off of Phoebe at some point in the past.

Its name comes from Norse mythology, where Thrymr is a Jotun or frost giant.

The name was said as Thrym in IAU Circular 8177. However, the IAU Working Group on Planetary System Nomenclature later decided to add the nominative case ending -r to the root Thrym.

References 
 IAUC 7538: S/2000 S 7, S/2000 S 8, S/2000 S 9 2000 December 7 (discovery)
 MPEC 2000-Y15: S/2000 S 1, S/2000 S 2, S/2000 S 7, S/2000 S 8, S/2000 S 9 2000 December 19 (discovery and ephemeris)
 IAUC 8177: Satellites of Jupiter, Saturn, Uranus 2003 August 8 (naming the moon Thrym)
 IAUC 8471: Satellites of Saturn 2005 January 21 (correcting the name)

Saturn's moons
Aegir (moon)

Aegir or Saturn XXXVI (provisional designation S/2004 S 10) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 11, 2005.

Aegir is about 6 kilometres in diameter, and orbits Saturn at an average distance of 19,618,000 km in 1025.908 days, at an inclination of 167° to the ecliptic (140° to Saturn's equator), with an eccentricity of 0.237.

It was named in April 2007 after Ægir, a giant from Norse mythology, the personification of tranquil seas, the one who soothes storms away. He is a son of Fornjót, and brother of Logi (fire, flame) and Kári (wind).

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn May 4 2005 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn May 3 2005 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (naming the moon)

Saturn's moons
S/2007 S 3

S/2007 S 3 is an unnamed moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 1, 2007, from observations taken between January 18 and April 19, 2007.

S/2007 S 3 is about 5 kilometres in diameter, and orbits Saturn at an average distance of 20,518,500 kilometres in about 1100 days, at an inclination of 177.22° to the ecliptic, with an eccentricity of 0.130.

References 
 Institute for Astronomy Saturn Satellite Data
 MPEC 2007-J09: S/2007 S 2, S/2007 S 3 May 1 2007 (discovery and ephemeris)
 IAUC 8836: S/2007 S 1, S/2007 S 2, and S/2007 S 3 (subscription-only) May 11 2007 (discovery)

Saturn's moons
Porrentruy (district)

The District of Porrentruy is one of the districts of the canton of Jura, Switzerland. The capital city is Porrentruy. The French-speaking district has a population of 24,012 (end of 2005).

Porrentruy is divided into 36 municipalities:

Districts of Jura
Franches-Montagnes (district)

The District of Franches-Montagnes is a district of the canton of Jura, Switzerland. The capital city is Saignelégier. The French-speaking district has a population of 9,865 (end of 2005).

Franches-Montagnes contains 19 municipalities:

Districts of Jura
Bestla (moon)

Bestla or Saturn XXXIX (provisional designation S/2004 S 18) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 13, 2004, and March 5, 2005.

Bestla is about 7 kilometres in diameter, and orbits Saturn at an average distance of 19,959,000 km in 1052.722 days, at an inclination of 147° to the ecliptic (151° to Saturn's equator), with an eccentricity of 0.772. This moon has the most eccentric orbit of any moon in the solar system.

It was named in April 2007 after Bestla, a frost giantess (female giant) from Norse mythology, mother of Odin.

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn May 4, 2005 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn May 3, 2005 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (naming the moon)

Saturn's moons
S/2004 S 7

S/2004 S 7 is an unnamed moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 8, 2005.

S/2004 S 7 is about 6 kilometres in diameter, and orbits Saturn at an average distance of 20,577,000 km in 1101.989 days, at an inclination of 166° to the ecliptic (166° to Saturn's equator), with an eccentricity of 0.554.

References
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn 2005 May 4 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn 2005 May 3 (discovery and ephemeris)

Saturn's moons
Beckenried

Beckenried is a municipality of the canton of Nidwalden in Switzerland. 

The main sights of Beckenried are: the church St. Heinrich and its cemetery chapel, the Ridli chapel, the chapel St. Anna, the Klewen chapel, fun fair (Älplerkilbi), and the St. Nikolas market.

References

Other websites
Official Homepage of Beckenried

Municipalities of Nidwalden
Buochs

Buochs is a municipality in the canton of Nidwalden in Switzerland. 

The main sights of Buochs are the church St. Martin, the Loreto chapel in Ennerberg, a monument of Johann Melchior Wyrsch, and the quay.

References

Other websites
Official Homepage of Buochs 

Municipalities of Nidwalden
S/2006 S 3

S/2006 S 3 is an unnamed moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on June 26, 2006, from observations taken between January and April 2006.

S/2006 S 3 is about 6 kilometres in diameter, and orbits Saturn at an average distance of 21,076,300 km in 1142.366 days, at an inclination of 150.8° to the ecliptic (128.8° to Saturn's equator), with an eccentricity of 0.4710.

References 
 Institute for Astronomy Saturn Satellite Data
 IAUC 8727: Satellites of Saturn 2006 June 30 (discovery)
 MPEC 2006-M45: Eight New Satellites of Saturn 2006 June 26 (discovery and ephemeris)

Saturn's moons
Fenrir (moon)

Fenrir is also a mythical creature from Norse mythology
Fenrir or Saturn XLI (provisional designation S/2004 S 16) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 13, 2004, and March 5, 2005.

Fenrir is about 4 kilometres in diameter, and orbits Saturn at an average distance of 22,611,000 km in 1269.362 days, at an inclination of 163° to the ecliptic (143° to Saturn's equator), with an eccentricity of 0.131.

It was named in April 2007 after Fenrisulfr, a giant wolf from Norse mythology, father of Hati and Skoll, son of Loki, destined to break its bonds for Ragnarök.

Other websites 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn May 4 2005 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn May 3, 2005 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (naming the moon)

Saturn's moons
Surtur (moon)

Surtur or Saturn XLVIII (also known as S/2006 S 7) is a moon of Saturn. It was discovered by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on June 26, 2006.

Surtur is about 6 kilometres in diameter, and orbits Saturn at an average distance of 22,243,600 km in 1238.575 days, at an inclination of 166.9° to the ecliptic (148.9° to Saturn's equator), with an eccentricity of 0.3680.

It was named in April 2007, after Surtr, leader of the fire giants of Norse mythology.

References
 Institute for Astronomy Saturn Satellite Data
 IAUC 8727: Satellites of Saturn 2006 June 30 (discovery)
 MPEC 2006-M45: Eight New Satellites of Saturn 2006 June 26 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (Naming the moon)

Saturn's moons
Kari (moon)

Kari or Saturn XLV (provisional designation S/2006 S 2) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on June 26, 2006, from observations taken between January and April 2006.

Kari is about 7 kilometres in diameter, and orbits Saturn at an average distance of 22,305,100 km in 1243.71 days, at an inclination of 148.4° to the ecliptic (151.5° to Saturn's equator), with an eccentricity of 0.3405.

It was named in April 2007 after Kári, son of Fornjót, the personification of wind in Norse mythology.

References 
 Institute for Astronomy Saturn Satellite Data
 IAUC 8727: Satellites of Saturn 2006 June 30 (discovery)
 MPEC 2006-M45: Eight New Satellites of Saturn 2006 June 26 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (Naming the moon)

Saturn's moons
Ymir (moon)

Ymir ( ), or Saturn XIX is a moon of Saturn. It was found by Brett J. Gladman, et al. in 2000, and given the designation S/2000 S 1. It was named in August 2003, from Norse mythology, where Ymir is the ancestor of all the Jotuns or frost giants.

Ymir is about 16 kilometres in diameter, and orbits Saturn at an average distance of 23,175,000 km in 1317.137 days, at an inclination of 172° to the ecliptic (146° to Saturn's equator), with an eccentricity of 0.358.

References 

 IAUC 7512: S/2000 S 1 and S/2000 S 2 2000 October 25 (discovery)
 MPEC 2000-Y15: S/2000 S 1, S/2000 S 2, S/2000 S 7, S/2000 S 8, S/2000 S 9 2000 December 19 (discovery and ephemeris)
 IAUC 8177: Satellites of Jupiter, Saturn, Uranus 2003 August 8 (naming the moon)

Other websites

 MPEC 2000-Y15: S/2000 S 1, S/2000 S 2, S/2000 S 7, S/2000 S 8, S/2000 S 9 (2000 Dec. 19 ephemeris)
 Ephemeris IAU-NSES
 Saturn's Known Satellites (by Scott S. Sheppard)

Saturn's moons
Loge (moon)

Loge or Saturn XLVI (provisional designation S/2006 S 5) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on June 26, 2006, from observations taken between January and April 2006.

Loge is about 6 kilometres in diameter, and orbits Saturn at an average distance of 23,142,000 km in 1314.364 days, at an inclination of 166.5° to the ecliptic (165.3° to Saturn's equator), with an eccentricity of 0.1390.

It was named in April 2007, after Loge (also spelled Logi), a fire giant from Norse mythology, son of Fornjót, sometimes confused with the god Loki.

References 
 Institute for Astronomy Saturn Satellite Data
 IAUC 8727: Satellites of Saturn 2006 June 30 (discovery)
 MPEC 2006-M45: Eight New Satellites of Saturn 2006 June 26 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (Naming the moon)

Saturn's moons
Fornjot (moon)

Fornjot or Saturn XLII (provisional designation S/2004 S 8) is a moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 11, 2005.

It is about 6 kilometres in diameter, and orbits Saturn at an average distance of 24,505,000 km in 1432 days at an inclination of 168° to the ecliptic (152° to Saturn's equator) with an eccentricity of 0.186. It is the farthest moon from Saturn.

It was named in April 2007, after Fornjót, a storm giant from Norse mythology, father of Ægir, Kári, and Loge.

References 
 Institute for Astronomy Saturn Satellite Data
 Jewitt's New Satellites of Saturn page
 IAUC 8523: New Satellites of Saturn May 4 2005 (discovery)
 MPEC 2005-J13: Twelve New Satellites of Saturn May 3, 2005 (discovery and ephemeris)
 IAUC 8826: Satellites of Jupiter and Saturn (subscription-only) 2007 April 5 (Naming the moon)

Saturn's moons
Cordelia (moon)

{{Infobox Planet
| name = Cordelia| image = File:Uranus rings and two moons.jpg
| caption = Cordelia (lower-middle, inside of bright ring), as imaged by Voyager 2
| bgcolour = #ffc0c0

| discoverer = Richard J. Terrile / Voyager 2
| discovered = January 20, 1986
| mean_orbit_radius = 49751.722 ± 0.149 km
| eccentricity = 0.00026 ± 0.000096
| period = 0.33503384 ± 0.00000058 d
| inclination = 0.08479 ± 0.031° (to Uranus' equator)
| satellite_of = Uranus

| dimensions = 50 × 36 × 36 km
| mean_radius = 21 ± 3 km
| surface_area = ~5500 km²
| volume = ~38,900 km³
| mass = ~5.0 kg
| density = ~1.3 g/cm³ assumed
| surface_grav = ~0.0073 m/s²
| escape_velocity = ~0.017 km/s
| rotation = synchronous
| axial_tilt = zero
| albedo = 0.08 ± 0.01
| single_temperature = ~64 K
}}Cordelia it the closest moon to Uranus.  It was found from the images taken by Voyager 2 on January 20, 1986, and was given the designation S/1986 U 7. It was not seen again until the Hubble Space Telescope observed it in 1997. Cordelia takes its name from the youngest daughter of Lear in William Shakespeare's King Lear. It is also designated Uranus VI'''. This moon is  wide and is the same size of Mars' smallest moon called Deimos.

Other websites
Cordelia Profile  by NASA's Solar System Exploration

Uranus' moons
Leberkäse

is a meat specialty. Other names include Leberkäs, Leberka(a)sand Fleischkäse. It originally was from the South of Germany. It can also be found in Austria and Switzerland. It is similar to meatloaf. It is made of corned beef, sometimes pork, bacon and onions. The ingredients are ground until they are very fine. They are then packed together into loaves. These are baked in an oven, until they get a brown crust.

Etymology
The word "Leberkäse" literally translates to "liver-cheese". In Bavaria there is neither cheese nor liver in the dish, though. Some linguists say, that the word may be related to the German word Laib (loaf). Perhaps it also contains the Slavic root quas (yeast).

What can be in Leberkäse
According to German food laws, only products called "Bavarian Leberkäse" are allowed not to have liver in them; otherwise, there must be a minimum liver content of 4%. Some local variants must contain even more liver; for example, the liver content of "Stuttgarter Leberkäse" must be at least 5%.

Eating Leberkäse

There are several ways of eating Leberkäse:
Cut into approximately finger-thick slices which are then placed in a semmel while still hot and seasoned with mustard. The result, generally called Leberkässemmel, is a staple of Bavarian and Austrian fast food restaurants.

Alternatively, the slices can also be pan-fried ("abgebräunt", browned), in which case they are commonly accompanied by a fried egg and German potato salad. This is a very common Biergarten dish sometimes called Strammer Max.  
 		 
Cold Leberkäse can also be cut into very thin slices and be used on a variety of sandwiches.

References

Other websites 
Bavarian Leberkäse 

Meat dishes
Albula (district)

Albula is one of the districts in the canton of Graubünden in Switzerland. It has an area of 723.13 km² and a population of 8,720 people (as of December 2004). 

Albula contains 4 Kreise (sub-districts) Alvaschein, Belfort, Bergün and Surses, which contains 23 municipalities:

Districts of Graubünden
Bernina (district)

Bernina  is a district in the canton of Graubünden, Switzerland. It has an area of 237.2 km² and a population of 4,687 people (as of December 2004).

Bernina consists of two Kreise (sub-districts) Brusio and Poschiavo, each of which contains a single municipality of the same name.

Districts of Graubünden
Ophelia (moon)

Ophelia is a closer moon of Uranus. It was found from the images taken by Voyager 2 on January 20, 1986, and was given the designation S/1986 U 8. It was not seen until the Hubble Space Telescope saw it in 2003.

Ophelia was named after the daughter of Polonius, Ophelia, in William Shakespeare's play Hamlet. It is also designated Uranus VII.

Unfortunately, other than its orbit, radius of 23 km and geometric albedo of 0.08, almost nothing is known about it. At the Voyager 2 images Ophelia appears as a streched object, the major axis pointing towards Uranus.

Other websites 
 Ophelia Profile  by NASA's Solar System Exploration

Uranus' moons
Hinterrhein (district)

Hinterrhein is a district of the canton of Graubünden, Switzerland. It has an area of 617.67 km² and a population of 12,508 people (as of December 2004). 

Hinterrhein consists of five Kreise (sub-districts) and 39 municipalities.

On 1 January 2006, Medels im Rheinwald became part of Splügen.

On 1 January 2003, the municipalities of Donath and Patzen-Fardün became part of Donat.

Districts of Graubünden
Imboden (district)

Imboden is a district of the canton of Graubünden, Switzerland. It has an area of 203.78 km² and a population of 17,528 people. (as of December 2004). 

It contains 2 Kreise (sub-districts) and seven municipalities:

Districts of Graubünden
Inn (district)

Inn is a district of the canton of Graubünden, Switzerland. It has an area of 1,196.77 km² and a population of 9,371 people (as of December 2004). 

It contains 4 Kreise (sub-districts) and 18 municipalities:

Districts of Graubünden
Landquart (district)

Landquart is a district of the canton of Graubünden, Switzerland. It has an area of 193.91 km² and a population of 22,450 people as of December 2004.

It contains 2 Kreise (sub-districts) and 11 municipalities

Sources 

Districts of Graubünden
Maloja (district)

Maloja  () is a district of the canton of Graubünden, Switzerland. It has an area of  and a population of 17,810 people (as of December 2004). Most of the population of Maloja speaks Italian.

It contains 2 Kreise (sub-districts) and 16 municipalities:

Districts of Graubünden
Moesa (district)

Moesa is a district of the canton of Graubünden, Switzerland. It has an area of 496.11 km² and a population of 7,640 people (as of December 2004). 

It contains 3 Kreise (sub-districts) and 17 municipalities:

Districts of Graubünden
Plessur (district)

Plessur is a district of the canton of Graubünden, Switzerland. It has an area of 266.73 km² and a population of 38,899 people (as of December 2004). The district is named after the river Plessur which crosses it. 

Plessur contains 3 Kreise (sub-districts) Chur, Churwalden and Schanfigg, which makes a total of 16 municipalities:

Districts of Graubünden
Davos (district)

Davos is a district of the canton of Graubünden, Switzerland. It has an area of 823.95 km² and a population of 25,728 people (as of December 2004). 

It contains 7 Kreise (sub-districts) and 16 municipalities:

The sub-districts Davos, Jenaz, Klosters, Küblis and Luzein belonged until 1986 to the defunct district Oberlandquart; the sub-districts Schiers and Seewis to the defunct district Unterlandquart.

Districts of Graubünden
Adrastea (moon)

Adrastea or , is the second closest moon to Jupiter. It was found by David C. Jewitt and G. Edward Danielson in Voyager 2 probe photographs taken in 1979 and received the designation . In 1983, it was named after the mythological Adrastea, who was a daughter of Jupiter and Ananke.

Adrastea was the first moon to be found from images taken by an interplanetary spacecraft, rather than through telescopic photography.

Physical characteristics 
Adrastea is non-spherical and measures 20x16x14 km³ across. What Adrastea is made of and the mass of Adrastea are not known, but assuming that its mean density is like that of Amalthea (~0.86 g/cm³) its mass can be estimated at ~2×1015 kg. Amalthea's density implies that moon is composed of water ice with a porosity of 10-15%, and Adrastea may be similar.

No surface details of Adrastea are known, due to the low resolution of available images.

Orbit 
Adrastea is the smallest and second closest member of the closer moons to Jupiter. It orbits Jupiter at ~129,000 km (1.806 Jupiter radii) within the planet's Main Ring. The orbital eccentricity of ~0.0015 and inclination of ~ 0.03° relative to the equator of Jupiter are very small.

Exploration 
Adrastea was found in Voyager 1 and 2 images, but appeared only as a dot. The Galileo spacecraft was able to see its shape, but the images remain poor.

References

Other websites 
 Adrastea Profile  by NASA's Solar System Exploration

Jupiter's moons
Surselva (district)

Surselva is a district of the canton of Graubünden, Switzerland. It has an area of 1,373.39 km² and a population of 22,381 people (as of December 2004).

It contains 5 Kreise (sub-districts) and 43 municipalities:

Districts of Graubünden
Almens

Almens is a municipality in the district of Hinterrhein in the Swiss canton of Graubünden. On 1 January 2015 the former municipalities of Almens, Paspels, Pratval, Rodels and Tomils merged into the new municipality of Domleschg.

Languages 
German is the most common language in Almens.

Other websites 

Official Web site

Former municipalities of Graubünden
Bernese Jura

Bernese Jura (German:Berner Jura, French: Jura Bernois) is a part of the canton of Bern in Switzerland. It is the French speaking part of the canton. It was made after the canton of Jura split from the canton of Bern. The Bernese Jura is made of three districts, Courtelary, La Neuveville and Moutier. The people living there are mainly protestants, they chose to stay with the canton of Bern in 1979.

Canton of Jura
Canton of Bern
Alvaneu

Alvaneu is a former municipality in the district of Albula in the canton of Graubünden in Switzerland.

It consists of Alvaneu-Dorf and Alvaneu-Bad. The area is 35.68 km² and the population is 421 people.

On 1 January 2015 the former municipalities of Alvaneu, Alvaschein, Brienz/Brinzauls, Mon, Stierva, Surava and Tiefencastel merged into the new municipality of Albula/Alvra.

Languages 
This table shows the languages of Alvaneu:

References

Other websites 

Gemeinde Alvaneu —official site of the municipality 
Bad Alvaneu—thermal baths 

Former municipalities of Graubünden
Birgisch

Birgisch was a municipality in the district of Brig in the canton of Valais in Switzerland.

On 1 January 2013 the former municipalities of Birgisch and Mund merged into the municipality of Naters.

Former municipalities of Valais
Amalthea (moon)

Amalthea is the third closest moon to Jupiter. It was found on September 9, 1892, by Edward Emerson Barnard and named after Amalthea, a nymph in Greek mythology. It is also known as .

On Amalthea, Jupiter would be an amazing sight in its sky, looking 92 times bigger than the Full Moon. Amalthea is the biggest of the closer moons of Jupiter. Non-spherical and reddish in colour, it is thought to have of water ice with unknown amounts of other materials. Its surface has big craters and high mountains.

Pictures of Amalthea were taken in 1979 and 1980 by the Voyager 1 and 2 spacecraft, and later, in more detail, by the Galileo orbiter in the 1990s.

Discovery and naming 
Amalthea was found on September 9, 1892 by Edward Emerson Barnard using the 36 inch (91 cm) telescope at Lick Observatory. It was the first new moon of Jupiter since Galileo Galilei's  discovery of the Galilean moons in 1610.

The moon is named after the nymph Amalthea from Greek mythology who nursed the infant Zeus (the Greek equivalent of Jupiter) with goat's milk. Its Roman numeral designation is . The name "Amalthea" was not adopted by the IAU until 1975, although it had been in use for many decades. The name was suggested by Camille Flammarion. Before 1975, Amalthea was most commonly known simply as . The adjectival form of the name is Amalthean.

Orbit 
Amalthea circles Jupiter at a distance of 181,000 km (2.54 Jupiter radii). The orbit of Amalthea has an eccentricity of 0.003 and an inclination of 0.37° relative to the equator of Jupiter.

Physical characteristics 
The surface of Amalthea is very red  The reddish color may be due to sulfur coming from Io or some other non ice material. Bright patches of green appear on the major slopes of Amalthea, but the nature of this color is currently unknown. The surface of Amalthea is a bit brighter than surfaces of other closer moons of Jupiter.

How Amalthea looks from Jupiter 

From Jupiter's surface —or rather, from just above its cloudtops— Amalthea would appear very bright, shining with a magnitude of −4.7, similar to that of Venus from Earth.

How Jupiter looks from Amalthea 
From the surface of Amalthea, Jupiter would look enormous: it would look 92 times bigger than the Full Moon.

Exploration 
In 1979-1980, the Voyager 1 and 2 spacecraft made the first images of Amalthea, which resolved its surface. They also measured the moon's surface temperature.  Later, the Galileo orbiter completed taking pictures of Amalthea's surface and a close flyby enabled it to constrain the moon's internal structure and composition.

References

Other websites 
 Amalthea Profile  by NASA's Solar System Exploration
 Another find for Galileo – Galileo Millennium Mission status report (2003-04-09)
 Jupiter's Amalthea Surprisingly Jumbled – JPL press release (2002-12-09)
 Jupiter From Amalthea, a painting by Frank Hettick, 2002.

Jupiter's moons
Eggerberg

Eggerberg is a municipality in the district of Brig in the canton of Valais in Switzerland.

References

Other websites
 Official website 

Municipalities of Valais
Mund

Mund was a municipality in the district of Brig in the canton of Valais in Switzerland.

On 1 January 2013 the former municipalities of Mund and Birgisch merged into the municipality of Naters.

Other websites
 Official website 

Former municipalities of Valais
Dallenwil

Dallenwil is a municipality in the canton of Nidwalden in Switzerland.

The main sights of Dallenwil are the ski and summer resort Wiesenberg/Wirzweli, the church St. Laurentius, and the pilgrimage chapel Wiesenberg.

References

Other websites 
  Dallenwil.ch   official website

Municipalities of Nidwalden
Emmetten

Emmetten is a municipality in the canton of Nidwalden in Switzerland. 

The main sights of Emmetten are the St. Anna chapel in Schöneck, the church St. Jakob und St. Theresia, the chapel of the holy cross with frescos of danse macabre in Sagendorf, and the chapel in Erlen.

References

Other websites
Official Homepage of Emmetten

Municipalities of Nidwalden
Ennetbürgen

Ennetbürgen is a municipality in the canton of Nidwalden in Switzerland.

The main sights of Ennetbürgen are the Saint Jost Chapel and the Church of Saint Anton.

References

Other websites
Official Homepage of Ennetbürgen

Municipalities of Nidwalden
Ennetmoos

Ennetmoos is a municipality in the canton of Nidwalden in Switzerland. 

The main sights of Ennetmoos are the chapels of  Saint Jakob, Saint Leonhard (in Rohren), and Saint Magnus (in Allweg), a monument (Überfalldenkmal) in Allweg, ruins at Rotzberg, the Stanserhorn mountain and resort, and the pilgrimage route St. Jakobsweg.

References

Other websites
Official Homepage of Ennetmoos

Municipalities of Nidwalden
Carpo (moon)

Carpo or , is a moon of Jupiter. It was found by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, and was designated as  until it got its name in early 2005.

Carpo is about 3 kilometres in diameter, and orbits Jupiter at an average distance of 17,145,000 km in 458.625 days, at an inclination of 56° to the ecliptic (55° to Jupiter's equator), and with an orbital eccentricity of 0.2736.
 
It was named in March 2005 after Carpo, one of the Horae, and a daughter of Zeus (Jupiter).

References 

Jupiter's moons
Sari

Sari () is the capital city of the Mazandaran province in Iran.

Cities in Iran
Rasht

Rasht  is the capital city of the Gilan province of Iran.

Cities in Iran
Mazandaran Province

Mazandaran (Persian: مازندران) is a province in the north of Iran. It is to the south of Caspian Sea. It has borders with Golestan, Semnan, Tehran, Qazvin and Gilan provinces.

References

Other websites 

Mazandaran
Kallichore (moon)

Kallichore or , is a moon of Jupiter. It was found by a team of astronomers from the University of Hawaii led by Scott S. Sheppard, et al. in 2003. It got the designation .

Kallichore is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 23,112,000 km in 717.806 days, at an inclination of 165° to the ecliptic (164° to Jupiter's equator), with an orbital eccentricity of 0.2042.

It was named in March 2005 after the nymph Kallichore.

Kallichore belongs to the Carme group, made up of non-spherical retrograde moons orbiting Jupiter at a distance ranging between 23,000,000 and 24,000,000 km and at an inclination of about 165°.

References 

Jupiter's moons
Eurydome (moon)

Eurydome or , is a moon of Jupiter. It was found by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2001, and given the designation .

Eurydome is about 3 kilometres in diameter, and orbits Jupiter at an average distance of 23,231,000 km in 723.359 days, at an inclination of 149° to the ecliptic (147° to Jupiter's equator), with an orbital eccentricity of 0.3770.

It was named in August 2003 after Eurydome in Greek mythology, who is sometimes described as the mother of the Graces by Zeus (Jupiter).

Eurydome belongs to the Pasiphaë group, non-spherical retrograde moons orbiting Jupiter at distances ranging between 22,800,000 and 24,100,000 km, and with inclinations ranging between 144.5° and 158.3°.

References 

Jupiter's moons
Sari (clothing)

A sari (also known as a saree or a shari) is a type of clothing for women. It is mostly used as a daily clothing in modern Republic of India, Bangladesh, Nepal and Sri Lanka as well as formal clothing in Pakistan. It is a very long strip of cloth. Women wrap it around their body. It is the National dress-code commonly worn by Bangladeshi and Indian women alike respectively. Also some Urdu or Mohajir-speaking communities of Pakistani women also wear this garment.

There are different kinds of saris for different occasions.

Gallery 

Clothing
Bangladeshi culture
Indian culture
National symbols of Bangladesh
National symbols of India
Thyone (moon)

Thyone or , is a non-spherical moon of Jupiter. It was found by a team of astronomers from the University of Hawaii led by Scott S. Sheppard, et al. in 2001, and given the designation .

Thyone is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 21,406,000 km in 639.803 days, at an inclination of 147° to the ecliptic (147° to Jupiter's equator) with an orbital eccentricity of 0.2526.

It was named in August 2003 after Thyone, better known as Semele, one of Zeus' conquests in Greek mythology.

Thyone belongs to the Ananke group, retrograde non-spherical moons which orbit Jupiter between 19,300,000 and 22,700,000 km, at inclinations of about 150°.

References 

Jupiter's moons
Sukhoi Su-27

The Su-27 Flanker is a Soviet/Russian single-seat fighter aircraft made by Sukhoi. It first flew on 20 May 1977, and was introduced on 23 August 1990. It was first made by the Soviet Union as a fighter, but now it is in the Russian Air Force. It can hold up to 10 guided Air-to-Air medium-range R-27E or short-range R-73 or unguided Air-to-Ground missiles, unguided bombs and a GSh-301 30mm cannon with 150 bullets. It has two AL-31F turbofan engines, a multi-purpose onboard search and track radar, an optical infrared search and track station with a laser rangefinder linked to pilot's helmet-mounted target designator and with a wide-angle HUD.

The Su-27 was made to pair with the MiG-29 Fulcrum, but in the Eritrean-Ethiopian War, Ethiopian Su-27s shot down 5 Eritrean MiG-29s. It was also supposed to fight American fighters like the F-15 Eagle and F-16 Fighting Falcon. There are the prototype versions T10 Flanker-A and T10S, the version S Flanker-B for the Russian Air Force, the interceptor version P Flanker-B without Air-to-Ground weapons for the Russian Air Force, the two-seat trainer version UB Flanker-C for the Russian Air Force, the export versions SK and UBK, the upgraded export versions SKM and UBM. There are fighters similar to the Su-27, like the Su-33 Flanker-D and the Su-30 Flanker-C .

The Su-27 is still in service with the Russian Air Force and others. Russian Air Force has hundreds of aircraft.
Half the fleet -about 100 fighters- has been modernized in the SM version from 2004 to 2012. The SM version has improved avionics, guided Air-to-Ground missiles and guided bombs and a “glass” cockpit. Russian Air Force received 12 newly built modernized SM3 aircraft in 2011.

Related pages
 MiG-29 Fulcrum
 F-16 Fighting Falcon
 F-15 Eagle
 F/A-18 Hornet
 F-14 Tomcat

References 

Indian military aircraft
Soviet military aircraft
Cold War
F. W. Murnau

Friedrich Wilhelm "F. W." Murnau (28 December 1888 – 11 March 1931) was a German movie director. He was one of the most influential directors of the silent movie era.  He was born in Bielefeld and attended the University of Heidelberg. He studied art history. He was openly gay. He was 6'4 (193 cm), He was said to have an icy disposition and an obsession with film. He was a combat pilot during World War I. He directed his first movie Der Knabe in Blau () in 1919.

Murnau's most famous movie is Nosferatu (1922). It was based on the book Dracula. Faust was Murnau's last German movie. Nosferatu and Faust were two of the first films to have original music. Some of his German movies were considered to be Expressionist movies.

Murnau went to Hollywood in 1926. He joined the Fox Studio. He made Sunrise in 1927. It did not make a lot of money. It did receive an Academy Award in 1929. Murnau's next two movies were sound movies. They were not well received. Murnau was disappointed. He quit Fox. He went to the South Pacific. In Bora Bora he made Tabu. The movie was censored in the United States for images of bare-breasted Polynesian women. Murnau died in an automobile accident in Santa Barbara, California. He is buried in Stahnsdorf near Berlin.

References

Other websites 

1888 births
1931 deaths
Gay men
German LGBT people
German military personnel of World War I
German movie directors
German movie producers
LGBT directors
People from North Rhine-Westphalia
Road accident deaths in California
Harpalyke (moon)

Harpalyke or , is a non-spherical moon of Jupiter. It was found by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2000, and given the designation . In August 2003,the moon was named after Harpalyke, the incestuous daughter of Klymenos, who was in some accounts a lover of Zeus (Jupiter).

Harpalyke belongs to the Ananke group, believed to be the remnants of a break-up of a captured asteroid. It is about 4 kilometres in diameter and appears grey similar to C-type asteroids. The moon orbits Jupiter at an average distance of 21,064,000 km in 624.542 days, at an inclination of 147° to the ecliptic (147° to Jupiter's equator) with an orbital eccentricity of 0.2441.

References 

 Ephemeris IAU-MPC NSES
 Mean orbital parameters NASA JPL

Other websites 
 David Jewitt pages
 Scott Sheppard pages

Jupiter's moons
Giganotosaurus

Giganotosaurus is a large theropod dinosaur. It lived during the Upper Cretaceous, about 10095 million years ago in what is now Argentina. 70 percent of the skeleton has been found. Giganotosaurus was probably the second largest carnivorous dinosaur of all time. Another large carnivore, Mapusaurus, also lived in the same territory. They were both relatives of the North African  Carcharodontosaurus. 

The largest specimen is  long, and 12.8 feet [3.9m] feet tall at the hip. Its weight is estimated as . 

Titanosaur fossils belonging to Andesaurus and Limaysaurus have been found near the remains of Giganotosaurus. The huge titanosaur Argentinosaurus also lived in the area. Probably, the titanosaurs were the main prey of the large theropods.

References 

Carnosaurs
Orthosie (moon)

Orthosie or , is a moon of Jupiter. It was found by a team of astronomers from the University of Hawaii led by Scott Sheppard in 2001, and given the designation .

Orthosie is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 20,568,000 km in 602.619 days, at an inclination of 142° to the ecliptic (143° to Jupiter's equator), with an orbital eccentricity of 0.2433.

It was named in August 2003 after Orthosie, the Greek goddess of prosperity and one of the Horae. The Horae (Hours) were daughters of Zeus and Themis.

Orthosie belongs to the Ananke group, retrograde non-spherical moons which orbit Jupiter between 19,300,000 and 22,700,000 km, at inclinations of about 150°.

References 

Jupiter's moons