2 Pallas
Pallas ( minor-planet designation : 2 Pallas ) is the second asteroid to have been discovered (after Ceres ), and is one of the largest asteroids in the Solar System . With an estimated 7% of the mass of the asteroid belt , it is the third-most-massive asteroid, being 10–30% less massive than Vesta . [17] It is 512 kilometers (318 mi) in diameter, somewhat smaller than 4 Vesta . It is likely a remnant protoplanet .
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
152048 characters 14 sections 29 paragraphs 15 images 204 internal links 123 external links |
pallas 0.873 vesta 0.137 ceres 0.129 asteroid 0.115 occultation 0.080 1779 0.076 athena 0.072 asteroids 0.065 olbers 0.062 renazzo 0.060 object 0.050 magnitude 0.050 discovered 0.049 512 0.045 pixel 0.043 |
Pallas ( minor-planet designation : 2 Pallas ) is the second asteroid to have been discovered (after Ceres ), and is one of the largest asteroids in the Solar System . With an estimated 7% of the mass of the asteroid belt , it is the third-most-massive asteroid, being 10–30% less massive than Vesta . [17] It is 512 kilometers (318 mi) in diameter, somewhat smaller than 4 Vesta . It is likely a remnant protoplanet . |
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| 2017 |
149052 characters 14 sections 28 paragraphs 15 images 206 internal links 109 external links |
pallas 0.873 vesta 0.137 ceres 0.129 asteroid 0.115 occultation 0.080 1779 0.076 athena 0.072 asteroids 0.065 olbers 0.062 renazzo 0.060 object 0.050 magnitude 0.050 discovered 0.049 512 0.045 pixel 0.043 |
Pallas , minor-planet designation 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and is one of the largest asteroids in the Solar System . With an estimated 7% of the mass of the asteroid belt , it is the third-most-massive asteroid, being 10–30% less massive than Vesta . [15] It is 512 kilometers (318 mi) in diameter, somewhat smaller than Vesta. It is likely a remnant protoplanet . |
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| 2016 |
142468 characters 14 sections 27 paragraphs 13 images 200 internal links 102 external links |
pallas 0.874 vesta 0.140 ceres 0.132 asteroid 0.118 occultation 0.082 athena 0.073 asteroids 0.066 olbers 0.063 renazzo 0.061 object 0.051 magnitude 0.051 discovered 0.050 512 0.046 pixel 0.044 meteorites 0.043 |
Pallas , minor-planet designation 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and it is one of the largest asteroids in the Solar System . With an estimated 7% of the mass of the asteroid belt , it is the third-most-massive asteroid, being 10–30% less massive than Vesta . [14] It is 512 kilometers (318 mi) in diameter, somewhat smaller than Vesta. It is likely a remnant protoplanet . |
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| 2015 |
139498 characters 14 sections 27 paragraphs 13 images 195 internal links 91 external links |
pallas 0.874 vesta 0.140 ceres 0.132 asteroid 0.118 occultation 0.082 athena 0.074 asteroids 0.066 olbers 0.063 renazzo 0.061 object 0.051 magnitude 0.051 discovered 0.050 512 0.046 pixel 0.044 meteorites 0.043 |
Pallas , minor-planet designation 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and it is one of the largest asteroids in the Solar System . With an estimated 7% of the mass of the asteroid belt , it is the third-most-massive asteroid, being 10–30% less massive than Vesta . [14] It is 512 kilometers (318 mi) in diameter, somewhat smaller than Vesta. It is likely a remnant protoplanet . |
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| 2014 |
128229 characters 10 sections 25 paragraphs 11 images 167 internal links 88 external links |
pallas 0.834 palladian 0.155 ceres 0.149 vesta 0.142 asteroid 0.133 asteroids 0.085 athena 0.083 olbers 0.071 renazzo 0.069 dawn 0.068 object 0.058 magnitude 0.057 discovered 0.050 pixel 0.049 meteorites 0.049 |
Pallas , minor-planet designation 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and it is one of the largest asteroids in the Solar System . It is estimated to comprise 7% of the mass of the asteroid belt , [14] and its diameter of 544 kilometres (338 mi) is slightly larger than that of 4 Vesta . It is 10–30% less massive than Vesta, [7] placing it third among the asteroids. It is likely a remnant protoplanet . |
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| 2013 |
126524 characters 10 sections 25 paragraphs 10 images 168 internal links 89 external links |
pallas 0.825 palladian 0.164 ceres 0.158 vesta 0.151 asteroid 0.121 athena 0.088 asteroids 0.079 olbers 0.075 renazzo 0.073 dawn 0.072 object 0.061 magnitude 0.061 discovered 0.053 pixel 0.052 meteorites 0.052 |
Pallas , minor-planet designation 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and one of the largest in the Solar System . It is estimated to comprise 7% of the mass of the asteroid belt , [13] and its diameter of 544 kilometres (338 mi) is slightly larger than that of 4 Vesta . It is however 10–30% less massive than Vesta, [6] placing it third among the asteroids. It is possibly the largest irregularly shaped body in the Solar System (that is, the largest body not rounded under its own gravity ) [ not verified in body ] , and a remnant protoplanet . |
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| 2012 |
126584 characters 10 sections 25 paragraphs 10 images 166 internal links 89 external links |
pallas 0.832 palladian 0.162 ceres 0.155 vesta 0.149 asteroid 0.119 athena 0.087 asteroids 0.078 olbers 0.074 renazzo 0.072 object 0.060 magnitude 0.060 dawn 0.053 discovered 0.052 pixel 0.052 meteorites 0.051 |
Pallas , minor-planet designation 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and one of the largest in the Solar System . It is estimated to comprise 7% of the mass of the asteroid belt , [13] and its diameter of 544 kilometres (338 mi) is slightly larger than that of 4 Vesta . It is however 10–30% less massive than Vesta, [6] placing it third among the asteroids. It is possibly the largest irregularly shaped body in the Solar System (that is, the largest body not rounded under its own gravity ) [ not verified in body ] , and a remnant protoplanet . |
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| 2011 |
119147 characters 10 sections 25 paragraphs 10 images 166 internal links 69 external links |
pallas 0.826 palladian 0.165 ceres 0.158 vesta 0.151 asteroid 0.121 athena 0.088 asteroids 0.079 olbers 0.076 renazzo 0.073 object 0.061 magnitude 0.061 dawn 0.054 discovered 0.053 pixel 0.053 meteorites 0.052 |
Pallas , formally designated 2 Pallas , is the second asteroid to have been discovered (after Ceres ), and one of the largest. It is estimated to comprise 7% of the mass of the asteroid belt , [13] and its diameter of 530 kilometres (330 mi)-565 kilometres (351 mi) is comparable to, or slightly larger than, that of 4 Vesta . It is however 20% less massive than Vesta, [6] placing it third among the asteroids. It is possibly the largest irregularly shaped body in the Solar System (that is, the largest body not rounded under its own gravity ) [ not verified in body ] , and a remnant protoplanet . |
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| 2010 |
114177 characters 10 sections 24 paragraphs 10 images 164 internal links 64 external links |
pallas 0.854 ceres 0.137 palladian 0.127 vesta 0.113 asteroid 0.107 asteroids 0.087 athena 0.085 olbers 0.073 renazzo 0.070 object 0.059 magnitude 0.059 hubble 0.056 dawn 0.052 pixel 0.051 meteorites 0.050 |
Pallas , formally designated 2 Pallas , is the second asteroid to have been discovered, by astronomer Heinrich Wilhelm Matthäus Olbers on March 28, 1802. It was at first considered a planet, as were other early asteroids, until the discovery of many more led to their re-classification. Pallas appears to be the largest irregularly shaped body in the Solar System (that is, the largest body not rounded under its own gravity), and a remnant protoplanet . |
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| 2009 |
110318 characters 10 sections 22 paragraphs 9 images 159 internal links 57 external links |
pallas 0.841 ceres 0.157 vesta 0.134 palladian 0.131 asteroid 0.110 asteroids 0.101 athena 0.087 olbers 0.075 renazzo 0.072 object 0.061 magnitude 0.061 hubble 0.058 dawn 0.054 pixel 0.052 meteorites 0.052 |
2 Pallas is the second asteroid to have been discovered, by astronomer Heinrich Wilhelm Matthäus Olbers on March 28, 1802. Pallas was at first considered a planet, as were the other early asteroids 1 Ceres , 3 Juno , and 4 Vesta , until the discovery of many additional asteroids led to their re-classification. It appears to be the largest irregularly shaped body in the Solar System, not completely rounded under its own gravity. |
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| 2008 |
98908 characters 7 sections 20 paragraphs 5 images 175 internal links 48 external links |
pallas 0.823 palladian 0.172 ceres 0.149 vesta 0.141 asteroid 0.127 asteroids 0.119 athena 0.092 olbers 0.079 renazzo 0.076 object 0.064 magnitude 0.064 hubble 0.061 dawn 0.057 pixel 0.055 meteorites 0.055 |
2 Pallas ( Template:PronEng PAL -əs , or as [ Παλλάς] error: {{lang-xx}}: text has italic markup ( help ) ) is one of the largest asteroids and is located in the main asteroid belt . It was the second asteroid to be discovered, by astronomer Heinrich Wilhelm Matthäus Olbers on March 28 , 1802 . Pallas was at first considered a planet, as were the other early asteroids 1 Ceres , 3 Juno , and 4 Vesta , until the discovery of many additional asteroids led to their re-classification. |
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| 2007 |
79564 characters 7 sections 20 paragraphs 3 images 160 internal links 32 external links |
pallas 0.839 asteroid 0.177 ceres 0.138 vesta 0.111 athena 0.097 object 0.090 olbers 0.083 renazzo 0.080 asteroids 0.075 palladian 0.072 magnitude 0.067 dawn 0.059 belt 0.058 inclination 0.057 meteorites 0.057 |
2 Pallas ( Template:PronEng , [ Παλλάς] error: {{lang-xx}}: text has italic markup ( help ) ) is an asteroid located in the asteroid belt region of the solar system and was the second to be discovered. It was found and named by astronomer Heinrich Wilhelm Matthäus Olbers on March 28 , 1802 . The adjectival form of the name is Palladian. |
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| 2006 |
31269 characters 8 sections 13 paragraphs 3 images 146 internal links 9 external links |
pallas 0.789 palladian 0.152 asteroid 0.139 vesta 0.116 occultation 0.113 belt 0.098 uncertainty 0.095 renazzo 0.084 παλλάς 0.084 əs 0.084 axial 0.078 greek 0.077 pal 0.076 cr 0.076 matthäus 0.076 |
Template:Minor Planet 2 Pallas (pal'-əs ( key ), Greek Παλλάς) is an asteroid located in the asteroid belt region of the solar system and was the second to be discovered. It was found and named by astronomer Heinrich Wilhelm Matthäus Olbers on March 28 , 1802 . Pallas is the third most massive object in the asteroid belt and is estimated to contain 7% of the region's entire mass. |
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| 2005 |
27688 characters 7 sections 16 paragraphs 1 images 138 internal links 8 external links |
pallas 0.757 palladian 0.165 asteroid 0.126 occultation 0.123 uncertainty 0.103 renazzo 0.091 παλλάς 0.091 axial 0.085 vesta 0.084 greek 0.084 pal 0.082 cr 0.082 neptunian 0.082 ceres 0.079 template 0.077 |
Template:Minor Planet 2 Pallas ( pal'-us , Greek Παλλάς ) was the first asteroid discovered after 1 Ceres . It was found and named by H. Wilhelm Olbers on March 28 , 1802 . It is estimated that it contains 9% of the mass of the entire main asteroid belt. |
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| 2004 |
11000 characters 1 sections 7 paragraphs 0 images 62 internal links 4 external links |
pallas 0.739 vesta 0.137 pal 0.134 occultation 0.133 ceres 0.129 template 0.126 speckle 0.126 asteroid 0.123 invariably 0.120 athena 0.120 wisdom 0.120 mythology 0.119 refuted 0.115 occulting 0.115 satellite 0.106 |
Template:Minor Planet 2 Pallas ("PAL us") was the first asteroid discovered after 1 Ceres . It was found and named by H. Wilhelm Olbers on March 28 , 1802 . It was named after Pallas of Greek mythology , the daughter of Triton and friend of Athena . There is another Pallas in Greek mythology who is male, the god of wisdom; however, the first asteroids were invariably given female names. |
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| 2003 |
3536 characters 0 sections 2 paragraphs 0 images 24 internal links 0 external links |
pallas 0.669 asteroid 0.335 wisdom 0.325 1802 0.286 olbers 0.279 noticeable 0.246 god 0.167 second 0.149 discovered 0.146 greek 0.123 circular 0.122 largest 0.085 orbit 0.059 2 0.041 named 0.027 |
2 Pallas is the second largest asteroid (and second asteroid discovered). Pallas was discovered (and named) by Olbers , in 1802 . Pallas was the Greek god of wisdom . The asteroid is noticeable for its nearly circular orbit . |
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| 2002 |
1733 characters 0 sections 1 paragraphs 0 images 10 internal links 0 external links |
1802 0.488 olbers 0.476 2nd 0.433 asteroid 0.381 pallas 0.381 largest 0.145 second 0.127 discovered 0.125 2 0.069 |