Bouvet triple junction

Up to 10 million years ago this third junction of the Mid-Atlantic Ridge and the two deep transform valleys of Conrad and Bouvet met in one point. Thus the triple junction was of the ridge-fault-fault (RFF) type.{{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} Conrad transform, known as the Conrad fracture zone,{{sfn|Sclater|Bowin|Hey|Hoskins|1976|p=1857}} stretching to the west, connected the end of the Mid-Atlantic Ridge to the South American-Antarctic Ridge. Bouvet transform, known as the Bouvet fracture zone,{{sfn|Sclater|Bowin|Hey|Hoskins|1976|p=1857}} linked it to the Southwest Indian Ridge on the eastern side,{{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} and this is known to be the oldest part of the current triple junction at 8 Ma.{{sfn|Buikin|Verchovsky|Migdisova|2018|p=1369}}

Up to 10 million years ago this third junction of the Mid-Atlantic Ridge and the two deep transform valleys of Conrad and Bouvet met in one point. Thus the triple junction was of the ridge-fault-fault (RFF) type.{{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} Conrad transform, known as the Conrad fracture zone,{{sfn|Sclater|Bowin|Hey|Hoskins|1976|p=1857}} stretching to the west, connected the end of the Mid-Atlantic Ridge to the South American-Antarctic Ridge. Bouvet transform, known as the Bouvet fracture zone,{{sfn|Sclater|Bowin|Hey|Hoskins|1976|p=1857}} linked it to the Southwest Indian Ridge on the eastern side,{{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} and this is known to be the oldest part of the current triple junction at 8 Ma.{{sfn|Buikin|Verchovsky|Migdisova|2018|p=1369}}

Currently the Conrad transform and Bouvet transform are no longer connected to each other. The Mid-Atlantic Ridge is retreating northward, at a rate of {{Convert|11|mm/year|abbr=on|in/year}}. New spreading sections of the South American-Antarctic Ridge and the Southwest Indian Ridge are growing northward from the eastern end of Conrad transform and the western end of Bouvet transform respectively, striving for the shifting triple point. Thus the Mid-Atlantic Ridge is opening like a [[zipper]]. The new spreading sections are somewhat unusual:

Currently the Conrad transform and Bouvet transform are no longer connected to each other. The Mid-Atlantic Ridge is retreating northward, at a rate of {{Convert|11|mm/year|abbr=on|in/year}}{{Citation needed|date=July 2025}}. New spreading sections of the South American-Antarctic Ridge and the Southwest Indian Ridge are growing northward from the eastern end of Conrad transform and the western end of Bouvet transform respectively, striving for the shifting triple point. Thus the Mid-Atlantic Ridge is opening like a [[zipper]]. The new spreading sections are somewhat unusual:

* One new spreading section of the South American-Antarctic Ridge is not perpendicular to Conrad fault, violating the perpendicular pattern of alternating spreading ridges and transform faults generally seen on slowly spreading oceanic ridges.

* One new spreading section of the South American-Antarctic Ridge is not perpendicular to Conrad fault, violating the perpendicular pattern of alternating spreading ridges and transform faults generally seen on slowly spreading oceanic ridges.

* The new part of the Southwest Indian Ridge is masked by the recently formed Spiess Seamount,{{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} which is also known as Spiess Ridge,{{sfn|Mitchell|Livermore|1998|p=15457}} and this means that it is not possible to classify the junction definitely as R-R-R as it may still be R-F-F transitioning to R-R-R, {{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} being for the last 1 Ma ridge–fault–ridge, (R-F-R).{{sfn|Buikin|Verchovsky|Migdisova|2018|p=1369}} This volcanic seamount is now more than 2 million years old,{{sfn|Buikin|Verchovsky|Migdisova|2018|p=1369}} and is the highest point in the area after Bouvet Island. Spiess Seamount was named after [[Captain (naval)|Captain]] {{ill|Fritz Spieß|de}} of the [[German Meteor expedition]] of 1926.{{sfn|Mitchell|Livermore|1998|p=15457}}

* The new part of the Southwest Indian Ridge is masked by the recently formed Spiess Seamount,{{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} which is also known as Spiess Ridge,{{sfn|Mitchell|Livermore|1998|p=15457}} and this means that it is not possible to classify the junction definitely as R-R-R as it may still be R-F-F transitioning to R-R-R, {{sfn|Mitchell|Livermore|Fabretti|Carrara|2000|p=8279}} being for the last 1 Ma ridge–fault–ridge, (R-F-R).{{sfn|Buikin|Verchovsky|Migdisova|2018|p=1369}} This volcanic seamount is now more than 2 million years old,{{sfn|Buikin|Verchovsky|Migdisova|2018|p=1369}} and is the highest point in the area after Bouvet Island. Spiess Seamount was named after [[Captain (naval)|Captain]] {{ill|Fritz Spieß|de}} of the [[German Meteor expedition]] of 1926.{{sfn|Mitchell|Livermore|1998|p=15457}}