The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were primordial objects leftover from the formation of Mars that were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] Another explanation involves asteroids chaotically wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the short dynamical lifetimes of these objects. [3] [4] The spectra of Eureka and two other Mars trojans indicates an olivine -rich composition. [5] Since olivine-rich objects are rare in the asteroid belt it has been suggested that some of the Mars trojans are captured debris from a large orbit-altering impact on Mars when it encountered a planetary embryo. [6] [3]
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
67143 characters 2 sections 6 paragraphs 5 images 266 internal links 25 external links |
trojans 0.481 eureka 0.332 yorp 0.283 lagrangian 0.238 l5 0.173 l4 0.171 objects 0.162 spinup 0.141 points 0.140 olivine 0.135 uj7 0.132 questionable 0.132 rotational 0.122 wandering 0.121 embryo 0.121 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were primordial objects leftover from the formation of Mars that were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] Another explanation involves asteroids chaotically wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the short dynamical lifetimes of these objects. [3] [4] The spectra of Eureka and two other Mars trojans indicates an olivine -rich composition. [5] Since olivine-rich objects are rare in the asteroid belt it has been suggested that some of the Mars trojans are captured debris from a large orbit-altering impact on Mars when it encountered a planetary embryo. [6] [3] |
|
2017 |
67162 characters 2 sections 6 paragraphs 5 images 265 internal links 25 external links |
trojans 0.413 eureka 0.343 yorp 0.291 lagrangian 0.246 l5 0.178 l4 0.176 objects 0.167 trojan 0.164 spinup 0.146 points 0.144 olivine 0.139 uj7 0.136 questionable 0.136 rotational 0.125 wandering 0.125 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were primordial objects leftover from the formation of Mars that were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] Another explanation involves asteroids chaotically wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the short dynamical lifetimes of these objects. [3] [4] The spectra of Eureka and two other Mars Trojan indicates an olivine-rich composition. [5] Since olivine-rich objects are rare in the asteroid belt it has been suggested that some of the Mars trojans are debris from a large impact on Mars that was captured when the orbit of Mars was altered when it encountered a planetary embryo. [6] [3] |
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2016 |
60999 characters 2 sections 5 paragraphs 5 images 264 internal links 17 external links |
trojans 0.546 lagrangian 0.406 points 0.238 questionable 0.225 wandering 0.206 asteroids 0.166 l5 0.147 l4 0.146 presently 0.140 trailing 0.132 considering 0.131 numerical 0.129 candidates 0.125 involves 0.123 candidate 0.121 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] One explanation for this involves asteroids wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the very low mass of Mars. [3] [4] |
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2015 |
62032 characters 2 sections 5 paragraphs 5 images 266 internal links 17 external links |
trojans 0.539 lagrangian 0.401 points 0.235 questionable 0.223 wandering 0.204 asteroids 0.164 cloud 0.154 l5 0.146 l4 0.144 presently 0.138 trailing 0.130 considering 0.129 numerical 0.127 candidates 0.124 involves 0.121 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] One explanation for this involves asteroids wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the very low mass of Mars. [3] [4] |
|
2014 |
61924 characters 2 sections 5 paragraphs 5 images 266 internal links 17 external links |
trojans 0.539 lagrangian 0.401 points 0.235 questionable 0.223 wandering 0.204 asteroids 0.164 cloud 0.154 l5 0.146 l4 0.144 presently 0.138 trailing 0.130 considering 0.129 numerical 0.127 candidates 0.124 involves 0.121 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] One explanation for this involves asteroids wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the very low mass of Mars. [3] [4] |
|
2013 |
61902 characters 2 sections 5 paragraphs 5 images 268 internal links 17 external links |
trojans 0.539 lagrangian 0.401 points 0.235 questionable 0.223 wandering 0.204 asteroids 0.164 cloud 0.154 l5 0.145 l4 0.144 presently 0.138 trailing 0.130 considering 0.129 numerical 0.127 candidates 0.124 involves 0.121 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that they were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case. [1] [2] One explanation for this involves asteroids wandering into the Mars Lagrangian points later in the Solar System's formation. This is also questionable considering the very low mass of Mars. [3] [4] |
|
2012 |
53750 characters 2 sections 5 paragraphs 4 images 266 internal links 7 external links |
trojans 0.537 lagrangian 0.400 candidates 0.247 points 0.235 questionable 0.222 wandering 0.203 asteroids 0.163 cloud 0.154 l5 0.145 citation 0.144 l4 0.143 presently 0.138 trailing 0.130 considering 0.129 involves 0.121 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. The origin of the Mars trojans is not well understood. One theory suggests that the Mars trojans were captured in its Lagrangian points as the Solar System was forming. However, spectral studies of the Mars trojans indicate this may not be the case [1] [2] . One explanation for this involves asteroids wandering into the Mars Lagrangian points later in the Solar System 's formation. This is also questionable considering the very low mass of Mars . [ citation needed ] |
|
2011 |
47996 characters 2 sections 4 paragraphs 4 images 259 internal links 1 external links |
l5 0.361 l4 0.357 presently 0.344 trojans 0.334 lagrangian 0.332 ahead 0.278 family 0.272 share 0.260 asteroids 0.203 points 0.195 60 0.177 objects 0.169 sun 0.132 group 0.100 orbit 0.095 |
The Mars trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. |
|
2010 |
13080 characters 2 sections 4 paragraphs 1 images 51 internal links 1 external links |
l5 0.361 l4 0.357 presently 0.344 trojans 0.334 lagrangian 0.332 ahead 0.278 family 0.272 share 0.260 asteroids 0.203 points 0.195 60 0.177 objects 0.169 sun 0.132 group 0.100 orbit 0.095 |
The Mars Trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. |
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2009 |
12457 characters 2 sections 4 paragraphs 1 images 49 internal links 1 external links |
l5 0.361 l4 0.357 presently 0.344 trojans 0.334 lagrangian 0.332 ahead 0.278 family 0.272 share 0.260 asteroids 0.203 points 0.195 60 0.177 objects 0.169 sun 0.132 group 0.100 orbit 0.095 |
The Mars Trojans are a group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead of and behind Mars. |
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2008 |
10926 characters 2 sections 3 paragraphs 0 images 48 internal links 1 external links |
presently 0.389 trojans 0.379 lagrangian 0.375 ahead 0.315 family 0.308 share 0.294 asteroids 0.230 points 0.220 consists 0.208 60 0.201 objects 0.192 sun 0.149 group 0.113 orbit 0.108 planet 0.082 |
Mars Trojans are a large group of objects that share the orbit of the planet Mars around the Sun . They can be found around the two Lagrangian points 60° ahead and behind of Mars. |