- Created on
- …
- Next Birthday
- …
- Last Active
- …
- Security Status
- 0.00
Combat Record
Career-long numbers from eve-kill
Combat
- Kills
- 1
- Losses
- 25
- Efficiency
- 4%
- Danger Ratio
- 100%
ISK
- Destroyed
- 0
- Lost
- 5.00B
- ISK Efficiency
- 0%
- Balance
- -5.00B
Solo
- Solo Kills
- 0
- Solo Ratio
- 0%
- Final Blows
- 0
- Points
- 1
Other
- NPC Losses
- 0
- NPC Loss Ratio
- 0%
- Avg Kills/Day
- —
- Activity
- Inactive
Damage
Damage Dealt257
Damage Taken25.2K
Damage Ratio1%
Combat profile
How they fight, with whom and against whom — last 90 days
Activity
What they fly and where they fight
Most Valuable
Matchups
Who they kill, who kills them, what they lose
Top ListsLast 90d
Hulls LostLast 90d
Losses broken down by hull class.
Career
Corporations flown for, most recent first
Imperial ShipmentSince Saturday, 14 June 20140 Kills1 Losses
Amok.Since Wednesday, 26 February 20140 Kills0 Losses
Imperial ShipmentSince Monday, 1 July 20130 Kills0 Losses
Trinity CouncilSince Tuesday, 20 November 20121 Kills12 Losses
Imperial ShipmentSince Tuesday, 19 July 20110 Kills10 Losses
First Flying Wing IncSince Tuesday, 12 July 20110 Kills0 Losses
Imperial ShipmentSince Sunday, 8 May 20110 Kills0 Losses
Flux Technologies IncSince Sunday, 1 May 20110 Kills0 Losses
Estel Arador Corp ServicesSince Saturday, 30 April 20110 Kills0 Losses
Isotech EngineeringSince Monday, 4 April 20110 Kills0 Losses
Imperial AcademySince Monday, 28 March 20110 Kills0 Losses
In-game bio
The hammerfall was a spherical shock wave of hydrogen plasma, blazing at a temperature of millions of degrees and compressed until it had many of the properties of metal. A hundred times as massive as the largest gas giant in the star system, by the time it slammed into the crystal of iron at the heart of the murdered star it was traveling at almost 2 percent of lightspeed. When it struck, a tenth of the gravitational potential energy of the star was converted into radiation in a matter of seconds. Fusion restarted, exotic reactions taking place as even the iron core began to soak up nuclei, building heavier and hotter and less stable intermediaries. In less than ten seconds, the star burned through a visible percentage of its fuel, enough to keep the fires banked for a billion years. There wasn't enough mass in the G-type dwarf to exceed the electron degeneracy pressure in its core, collapsing it into a neutron star...