Wormhole, Wormhole Size and Stability Information See the table below for a list of the restrictions for each wormhole type. These restrictions include The maximum amount of mass that is allowed to pass through them, the maximum mass that can pass though in a single jump, and the maximum time that the wormhole will remain open for. This effect is generally most visible at the moment a hole drops to 50% or 10% mass and thus actively shrinks, as it can be more difficult to get an idea of the wormhole's visible size in a vacuum.Every wormhole has certain restrictions that are determined by the wormhole type. With less than 4 hours left on the hole the aurora become faded and have less defined forms.įurthermore, as a wormhole becomes destabilized from large amounts of mass traversing it, it starts to shrink. With 24-4 hours left on the hole the aurora surrounding it wiggle more. This is the most important one to recognise as it will allow scouting frigate to pass through but deny the main fleet from jumping.Ī wormhole with a teal aurora allows medium sized ships, including cruisers, battlecruisers and industrials, to pass through (20,000,000 kg).Ī gray aurora highlights a wormhole that allows every ship below capital hulls to pass through (300,000,000 kg).Ī yellow aurora indicates wormholes that freighters and capitals can transit (1,000,000,000 kg, 1,350,000,000 kg or 1,800,000,000 kg).Īs the wormhole gets older the visuals change slightly. The color of the flare around a wormhole will tell you the maximum mass of ships that can go through.Ī royal blue aurora indicates wormholes that only allow frigate-mass ships (5,000,000 kg). Wormholes not only allow certain amounts of mass through them in their lifetime, but they also have mass restrictions for each particular transfer. Not all shattered wormholes have this visual. This skybox is shown on Thera wormholes, C13 frigate sized shattered wormholes and on Drifter wormholes. Some of the more unique wormhole systems also have their own skybox so it is possible to identify them visually without jumping. The region on the other side of the wormhole is Solitude. An experienced pilot can also identify various objects visible to make a more accurate estimation on the target system, in this particular image Cloud Ring is clearly visible. The green color indicates the wormhole leading into a Gallente region. Null regions are mostly black with smaller colored clouds. A red k-Space wormhole will most likely take you to a Minmatar region, yellow k-space connection to Amarr region, blue k-space wormhole to Caldari region and green k-space connection to Gallente region. Wormholes leading to k-Space also take the skybox of the region on the other side. Wormholes leading to class 6 are very chromatic orange with black details. The white cloud is not as bright as it in C4 connection. Wormholes leading to class 5 are again dark red but with some brown hues mixed in. The color of a wormhole to C4 system is unique making it easier to identify by color instead of shapes. Wormholes leading to class 4 are mainly dark red with one bright white cloud and some distinct black spots. The distinct red cloud easy to identify mark of a C3 connection. Wormholes leading to class 3 have again grayish clouds. The most notable feature of this skybox is the black spot in the light gray cloud. Wormholes leading to class 2 have a brownish hue with some gray clouds. A wormhole leading to C1 system may look similar to a wormhole leading to C2 or C3 system, the most notable difference is lack of any notable detail. Wormholes leading to class 1 systems have grayish clouds with some black spots and some blue and cyan details. Use the context menu in the overview to look at the wormhole and rotate the sphere in space using the mouse if the wormhole looks different than the pictures below. The visual representation of a wormhole in EVE Online is a sphere. The center eye of a wormhole will always take the skybox of the destination system This can be used to see what class wormhole system it leads to or what region it leads to.
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