Difference between revisions of "White Glaze Belt"

From EVE University Wiki
Jump to: navigation, search
(Redirected page to Ice harvesting#Ice belts)
(Replace redirect by a stub)
Tag: Removed redirect
Line 1: Line 1:
#redirect [[Ice harvesting#Ice belts]]
+
A White Glaze Belt is a [[Cosmic Anomaly]] found in High and Low Security Space in the [[Topology|Caldari quadrant]]. It can be [[Ice harvesting|mined]] with a properly fitted [[Mining Ships|mining ship]]. A White Glaze Belt can only be found in one of the ice systems (see below for the full list of High Sec and Low Sec systems).
 +
 
 +
While sharing the same name, the contents of a Glacial Mass Belt are different in High Sec, Low Sec higher than 0.1 and in Low Sec with security 0.1.
 +
 
 +
<!--[[File:White Glaze Belt.jpg|right|thumb|Ice quantity in lowsec.]]-->
 +
{| class="wikitable" style="width: 440px; text-align: center;" summary="Ore Summary Table"
 +
|-
 +
! scope="col" | Ore&nbsp;Type
 +
! scope="col" | # of Asteroids
 +
! scope="col" | Ore Quantity
 +
! scope="col" | m³ per Unit
 +
! scope="col" | m³ total
 +
 
 +
|-
 +
| style="text-align: left;" | White Glaze
 +
| ?| ?
 +
| 1,000
 +
| ?
 +
|-
 +
| style="text-align: left;" | Glare Crust (0.4 sec or less)
 +
| ?
 +
| ?
 +
| 1,000
 +
| ?
 +
|-
 +
| style="text-align: left;" | Dark Glitter (0.1 sec)
 +
| ?
 +
| ?
 +
| 1,000
 +
| ?
 +
|}
 +
{{IceNav}}
 +
{{Stub}}
 +
[[Category:Ice belts]]

Revision as of 05:55, 9 April 2024

A White Glaze Belt is a Cosmic Anomaly found in High and Low Security Space in the Caldari quadrant. It can be mined with a properly fitted mining ship. A White Glaze Belt can only be found in one of the ice systems (see below for the full list of High Sec and Low Sec systems).

While sharing the same name, the contents of a Glacial Mass Belt are different in High Sec, Low Sec higher than 0.1 and in Low Sec with security 0.1.

Ore Type # of Asteroids Ore Quantity m³ per Unit m³ total
White Glaze ? 1,000 ?
Glare Crust (0.4 sec or less) ? ? 1,000 ?
Dark Glitter (0.1 sec) ? ? 1,000 ?
This article is a stub. You can help the UniWiki by expanding it.