Wormhole Signature Strength List

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All this data is potentially out of date, and should be taken with a truckload of salt

The following resource lists the bands in which each type of wormhole appears. Pilots who know the possible wormholes which may appear in the system they are currently scouting, can speed their search for exits. Remember, only certain static wormholes will be possible, depending on what constellation the wormhole system lies within, thus, the other statics may be discounted (see List of All W-Space Systems):

Wormhole Signature Bands
Location 10.0%
(1/10 Band)
6.67%
(1/15 Band)
5.0%
(1/20 Band)
4.0%
(1/25 Band)
2.5%
(1/40 Band)
2.22%
(1/45 Band)
1.25%
(1/80 Band**)
Unknown
Band
all K162
generic exit
highsec
wandering
Z971
high c1
R943
high c2
X702
high c3
? (O128?)
high c4
M555
high c5
? (B041?)
high c6
B041****
high c6
A641
high high
R051
high low
V283
high null
O128
high c4
lowsec
wandering
X702
low c3
? (O128?)
low c4
Z971
low c1
R943
low c2
N432
low c5
? (U319?)
low c6
O128 c4
U319 c6
N944
low low
? (B449?)
low high
? (S199?)
low null
B449 high
S199 null
nullsec
wandering
N432
null c5
? (U319?)
null c6
X702
null c3
? (O128?)
null c4
Z971
null c1
R943
null c2
O128 c4
U319 c6
? (S199?)
null null
N944
null low
B449
null high
S199
null null
class 1
static
N110
c1 high
J244
c1 low
Z060
c1 null

wandering
H121
c1 c1
C125
c1 c2
O883
c1 c3
M609
c1 c4
L614
c1 c5
S804
c1 c6 **
class 2 static B274
c2 high
A239
c2 low
E545
c2 null
psudo-
static*
Z647
c2 c1
D382
c2 c2
O477
c2 c3
Y683
c2 c4
N062
c2 c5
R474
c2 c6
class 3
static
U210
c3 low
D845
c3 high
K346
c3 null

wandering
N968
c3 c3
T405
c3 c4
V301
c3 c1
I182
c3 c2
N770
c3 c5
A982
c3 c6
class 4
static
C247
c4 c3
X877
c4 c4
P060
c4 c1
N766
c4 c2
H900
c4 c5
U574
c4 c6 **
class 5
static
H296
c5 c5
V753
c5 c6
E175
c5 c4 ***
Y790
c5 c1
D364
c5 c2 **
M267
c5 c3 ***

wandering
Z142
c5 null
C140
c5 low
D792
c5 high
class 6
static
V911
c6 c5
W237
c6 c6
L477
c6 c3
Z457
c6 c4
Q317
c6 c1
G024
c6 c2 **

wandering
Z142
c6 null
C140
c6 low
D792
c6 high
The theoretical wormhole configurations below are all of unknown scope and unknown signature strength.
Not Yet Found S047
 ? high
B520
 ? high
N290
 ? low
C391
 ? low
C248
 ? null
K329
 ? null
*Publication on psudo-statics to come soon... until then, see this post.
**I suspect there was an error in the original data or the signature strengths have changed:
all wormholes in the 1/80 band should probably be in the newly discovered 1/45 band.
***M267 should probably be in the 1/20 band and E175 in the 1/25 band
****B041 might not form in high sec or is exceedingly rare: see Project Snapshot
This is a product of Project Atlas.

Some helpful hints for scanning these bands in Anoikis:
Class 1, 3, 5, and 6 wormhole systems have one static wormhole which is native to that system, and these systems may also see a number of wandering wormholes within various bands.
Class 2 systems have two static wormholes, one to k-space and one to w-space, the combination of which depends on which constellation they belong to. (see List of All W-Space Systems: Class 2 Wormhole Systems)
Class 2 and 4 systems have only static wormholes and K162s.
All classes of wormholes will see many K162s which are always in the 1/10 band.
Keep in mind, that a given system will only commonly see one static type, but from time to time an "extra" static type wormhole might appear (these are currently under study by Project Atlas and are theorized to be Constellation Statics).

Wormhole Attributes[edit]

The following charts contain indexing information for navigating wormhole probability space. These charts are constructed using detailed wormhole position data from Project Compass, w-space system/constellation/region information recorded by Brawyn78 at his datacore before the information became unreadable through the NeoCom (note: this information is once again available in the NeoCom), and wormhole signature strength and general location data gathered and shared by Elisa Fir. Note, these data are not yet complete some wormholes have never been seen to my knowledge (lifetime and mass data for undocumented wormholes is constructed from theoretical models and experimental verification may be required). Wandering (a.k.a. "periodic") wormhole counts come from Project Snapshot data.

Template:Wormhole attributes


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