(101429) 1998 VF31
(101429) 1998 VF 31 is a sub-kilometer asteroid that orbits near Mars 's L 5 Lagrangian point , on average trailing 60° behind it. Its orbit is highly stable, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
48851 characters 3 sections 2 paragraphs 5 images 229 internal links 13 external links |
5261 0.424 eureka 0.401 101429 0.240 achondrites 0.240 vf31 0.228 mesosiderite 0.219 spectroscopically 0.196 suggesting 0.185 l5 0.157 undergone 0.148 lagrangian 0.144 indicate 0.141 trailing 0.140 proportion 0.139 spectroscopic 0.139 |
(101429) 1998 VF 31 is a sub-kilometer asteroid that orbits near Mars 's L 5 Lagrangian point , on average trailing 60° behind it. Its orbit is highly stable, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
|
| 2017 |
46606 characters 3 sections 2 paragraphs 5 images 224 internal links 14 external links |
5261 0.427 eureka 0.404 101429 0.241 achondrites 0.241 vf31 0.230 mesosiderite 0.221 spectroscopically 0.197 suggesting 0.187 l5 0.158 undergone 0.149 lagrangian 0.145 indicate 0.142 trailing 0.141 proportion 0.140 spectroscopic 0.140 |
(101429) 1998 VF 31 is a small asteroid that orbits near Mars 's L 5 Lagrangian point , on average trailing 60° behind it. Its orbit is highly stable, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
|
| 2016 |
46606 characters 3 sections 2 paragraphs 5 images 224 internal links 14 external links |
5261 0.427 eureka 0.404 101429 0.241 achondrites 0.241 vf31 0.230 mesosiderite 0.221 spectroscopically 0.197 suggesting 0.187 l5 0.158 undergone 0.149 lagrangian 0.145 indicate 0.142 trailing 0.141 proportion 0.140 spectroscopic 0.140 |
(101429) 1998 VF 31 is a small asteroid that orbits near Mars 's L 5 Lagrangian point , on average trailing 60° behind it. Its orbit is highly stable, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
|
| 2014 |
40040 characters 3 sections 2 paragraphs 6 images 186 internal links 7 external links |
5261 0.427 eureka 0.404 101429 0.241 achondrites 0.241 vf31 0.230 mesosiderite 0.221 spectroscopically 0.197 suggesting 0.187 l5 0.158 undergone 0.149 lagrangian 0.145 indicate 0.142 trailing 0.141 proportion 0.140 spectroscopic 0.140 |
(101429) 1998 VF 31 is a small asteroid that orbits near Mars 's L 5 Lagrangian point , on average trailing 60° behind it. Its orbit is highly stable, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
|
| 2013 |
40536 characters 3 sections 2 paragraphs 6 images 194 internal links 7 external links |
5261 0.422 eureka 0.399 101429 0.238 achondrites 0.238 vf31 0.227 mesosiderite 0.218 spectroscopically 0.195 suggesting 0.184 lagrange 0.180 l5 0.156 undergone 0.147 indicate 0.140 trailing 0.140 proportion 0.139 spectroscopic 0.139 |
(101429) 1998 VF 31 is a small asteroid which orbits the L 5 point trailing 60° behind the orbit of Mars . It is in a highly stable orbit around the Martian Lagrange point, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
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| 2012 |
38552 characters 3 sections 3 paragraphs 5 images 188 internal links 7 external links |
5261 0.422 eureka 0.399 101429 0.238 achondrites 0.238 vf31 0.227 mesosiderite 0.218 spectroscopically 0.195 suggesting 0.184 lagrange 0.180 l5 0.156 undergone 0.147 indicate 0.140 trailing 0.140 proportion 0.139 spectroscopic 0.139 |
(101429) 1998 VF 31 is a small asteroid which orbits the L 5 point trailing 60° behind the orbit of Mars . It is in a highly stable orbit around the Martian Lagrange point, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
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| 2011 |
38552 characters 3 sections 3 paragraphs 5 images 188 internal links 7 external links |
5261 0.422 eureka 0.399 101429 0.238 achondrites 0.238 vf31 0.227 mesosiderite 0.218 spectroscopically 0.195 suggesting 0.184 lagrange 0.180 l5 0.156 undergone 0.147 indicate 0.140 trailing 0.140 proportion 0.139 spectroscopic 0.139 |
(101429) 1998 VF 31 is a small asteroid which orbits the L 5 point trailing 60° behind the orbit of Mars . It is in a highly stable orbit around the Martian Lagrange point, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
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| 2010 |
17515 characters 3 sections 2 paragraphs 2 images 45 internal links 5 external links |
5261 0.422 eureka 0.399 101429 0.238 achondrites 0.238 vf31 0.227 mesosiderite 0.218 spectroscopically 0.195 suggesting 0.184 lagrange 0.180 l5 0.156 undergone 0.147 indicate 0.140 trailing 0.140 proportion 0.139 spectroscopic 0.139 |
(101429) 1998 VF 31 is a small asteroid which orbits the L 5 point trailing on the Mars orbit 60° behind the Mars . It is in a highly stable orbit around the Martian Lagrange point, and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] |
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| 2009 |
16364 characters 3 sections 2 paragraphs 1 images 41 internal links 5 external links |
101429 0.393 vf31 0.374 5261 0.347 eureka 0.328 lagrange 0.297 achondrites 0.196 mesosiderite 0.180 1998 0.165 spectroscopically 0.160 suggesting 0.152 l5 0.128 newer 0.126 undergone 0.121 indicate 0.116 trailing 0.115 |
(101429) 1998 VF 31 is a small sized asteroid which orbits the L 5 Lagrange point trailing 60 ° behind Mars in its orbit. It is in a highly stable orbit around the Martian Lagrange point and was originally thought to be spectroscopically similar to 5261 Eureka , suggesting they may both be primordial Martian asteroids. [3] Newer specral measurements, however, reveal differeces differences in the spectra with 5261 Eureka, suggesting they may not be related to each other after all. [2] |