Doc Stonecutter
Sep 13, 2020
Aug 30, 2020(5y)
Aug 30, 2026(100d)
Combat
Kills3
Losses86
Efficiency3%
ISK
Destroyed12.53b
Lost12.04b
ISK Eff.51%
Solo
Solo Kills0
Solo Ratio0%
Final Blows0
Points3
Other
NPC Losses9
NPC Loss Ratio10%
Avg Kills/Day0.00
ActivityInactive
Doc Stonecutter
Last Active
Sep 13, 2020
Birthday
Aug 30, 2020 (5 years old)
Next Birthday
Aug 30, 2026 (100 days)
Combat
Kills3
Losses86
Efficiency3%
Danger Ratio90%
ISK
Destroyed12.53b
Lost12.04b
ISK Efficiency51%
Balance+487.38m
Solo
Solo Kills0
Solo Ratio0%
Final Blows0
Points3
Other
NPC Losses9
NPC Loss Ratio10%
Avg Kills/Day0.00
ActivityInactive
No data available
Bio
Sonter (2006) explains asteroid mining as the key to the future economy of space. The asteroids are, according to Sonter, the most cost-effective way to commercialize space, and about 10% of NEAs are energetically more accessible than the Moon, meaning that less energy is needed to visit them.
The asteroids we know of are debris from the formation process of planets and a part of a solar system's history (Matter et al. 2011; Andreic 2016). Their sizes, shapes, bulk densities and surface properties are all clues to how and when they were formed through collisional evolution.
The small asteroids have assumedly suffered less alteration through fewer collisions and have more conserved pristine material, which could be useful for a mining expedition.
There has existed observational methods for the solar systems for many millennia. However, asteroids have long been an understudied celestial phenomena; there were no sufficient methods or technology around that would do the job properly. It was, according to Kowal (1996) not until almost 1970 when individual asteroids could be analyzed in a more specific matter, such as contour, size and composition through remote sensing techniques. Now the asteroids are, for instance, a major part in the unsolved mysteries about the origin of a solar system. And precise observations could be a way of solving them. Through observing asteroids using modern methods described herein; information can be interpreted to gain knowledge of orbital position of an asteroid, the variation in texture of its surface, its shape and even rotation. By gaining information on these features and setting it into context with surrounding asteroids, it is possible to perform statistical analyses which could improve our
knowledge of the asteroids evolution and origin within a solar system (Kowal 1996).
-Vide Hellgren, Asteroid Mining: A Review of Methods and Aspects, 2016
-------------------\xd2w\xd3--------------------
I follow the THE NEW HALAIMA CODE OF CONDUCT.
Permit Holder: Doc Stonecutter Purchase date - expires: 05.07.2021 - 05.07.2022
Agent: Gay Pride BOOOOOM
http://www.minerbumping.com/p/the-code.html
Specific Non-AFK mining permit for decently fited barges
--------------WHAT'S THIS ?-----------------
The asteroids we know of are debris from the formation process of planets and a part of a solar system's history (Matter et al. 2011; Andreic 2016). Their sizes, shapes, bulk densities and surface properties are all clues to how and when they were formed through collisional evolution.
The small asteroids have assumedly suffered less alteration through fewer collisions and have more conserved pristine material, which could be useful for a mining expedition.
There has existed observational methods for the solar systems for many millennia. However, asteroids have long been an understudied celestial phenomena; there were no sufficient methods or technology around that would do the job properly. It was, according to Kowal (1996) not until almost 1970 when individual asteroids could be analyzed in a more specific matter, such as contour, size and composition through remote sensing techniques. Now the asteroids are, for instance, a major part in the unsolved mysteries about the origin of a solar system. And precise observations could be a way of solving them. Through observing asteroids using modern methods described herein; information can be interpreted to gain knowledge of orbital position of an asteroid, the variation in texture of its surface, its shape and even rotation. By gaining information on these features and setting it into context with surrounding asteroids, it is possible to perform statistical analyses which could improve our
knowledge of the asteroids evolution and origin within a solar system (Kowal 1996).
-Vide Hellgren, Asteroid Mining: A Review of Methods and Aspects, 2016
-------------------\xd2w\xd3--------------------
I follow the THE NEW HALAIMA CODE OF CONDUCT.
Permit Holder: Doc Stonecutter Purchase date - expires: 05.07.2021 - 05.07.2022
Agent: Gay Pride BOOOOOM
http://www.minerbumping.com/p/the-code.html
Specific Non-AFK mining permit for decently fited barges
--------------WHAT'S THIS ?-----------------
Dashboard
Stats
Kills0
Losses0
Efficiency0%
ISK Destroyed0
ISK Lost0
ISK Efficiency0%
Solo Kills0
Solo Losses0
NPC Losses0
Blob Factor0
Active TimezoneUSTZ
Final Blows0
Points0
Activity Heat Map (EVE Time)
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Intel Profile
PlaystyleSolo (0 kills)
Avg Fleet: -