Data

Drowned dolines - the blue holes of the Pompey Reefs, Great Barrier Reef

Australian Ocean Data Network
Backshall, D.G. ; Barnett, J. ; Davies, P.J. ; Duncan, D.C. ; Harvey, N. ; Hopley, D. ; Isdale, P.J. ; Jennings, J.N. ; Moss, R.
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=https://pid.geoscience.gov.au/dataset/ga/80991&rft.title=Drowned dolines - the blue holes of the Pompey Reefs, Great Barrier Reef&rft.identifier=https://pid.geoscience.gov.au/dataset/ga/80991&rft.publisher=Bureau of Mineral Resources, Geology and Geophysics&rft.description=Blue holes occur at Cockatoo and Molar Reefs, in the Pompey hard line reefs. These two holes are roughly circular in shape, between 240-295 m in diameter, and 30-40 m deep. They are completely (Cockatoo) or partially (Molar) rimmed by profuse living coral and surrounded by lagoonal depths of 5-10 m. The inner slopes of the Cockatoo blue hole are 60-70° down to a depth of 25 m, below which coalescing sediment fans markedly reduce this angle. At the Molar blue hole, slopes are mainly gentler (45°) and sediment fans and terraces occur below 16 m. Distinct biological/sedimentary associations occur in both holes. Seismic refraction studies across the rim of the blue holes show a shallow (8.5-11 m) pre-Holocene surface beneath the rims. The balance of evidence suggests that the blue holes represent collapsed dolines which may have taken more than one low sea-level period to form. The original surface structures have been modified by subaerial solution processes, and subsequent sediment infill and coral growth following the Holocene transgression.Maintenance and Update Frequency: unknownStatement: Unknown&rft.creator=Backshall, D.G. &rft.creator=Barnett, J. &rft.creator=Davies, P.J. &rft.creator=Duncan, D.C. &rft.creator=Harvey, N. &rft.creator=Hopley, D. &rft.creator=Isdale, P.J. &rft.creator=Jennings, J.N. &rft.creator=Moss, R. &rft.date=1979&rft.coverage=westlimit=150.0; southlimit=-21.75; eastlimit=152.0; northlimit=-20.25&rft.coverage=westlimit=150.0; southlimit=-21.75; eastlimit=152.0; northlimit=-20.25&rft_rights=&rft_rights=Creative Commons Attribution 4.0 International Licence&rft_rights=CC-BY&rft_rights=4.0&rft_rights=http://creativecommons.org/licenses/&rft_rights=WWW:LINK-1.0-http--link&rft_rights=Australian Government Security ClassificationSystem&rft_rights=https://www.protectivesecurity.gov.au/Pages/default.aspx&rft_rights=WWW:LINK-1.0-http--link&rft_rights=Creative Commons Attribution 4.0 International Licence http://creativecommons.org/licenses/by/4.0&rft_subject=geoscientificInformation&rft_subject=GA Publication&rft_subject=Journal&rft_subject=marine&rft_subject=QLD&rft_subject=EARTH SCIENCES&rft_subject=Published_External&rft.type=dataset&rft.language=English Access the data

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CC-BY

Creative Commons Attribution 4.0 International Licence
http://creativecommons.org/licenses/by/4.0

Creative Commons Attribution 4.0 International Licence

CC-BY

4.0

http://creativecommons.org/licenses/

WWW:LINK-1.0-http--link

Australian Government Security ClassificationSystem

https://www.protectivesecurity.gov.au/Pages/default.aspx

WWW:LINK-1.0-http--link

Access:

Open

Contact Information

clientservices@ga.gov.au

Brief description

Blue holes occur at Cockatoo and Molar Reefs, in the Pompey hard line reefs. These two holes are roughly circular in shape, between 240-295 m in diameter, and 30-40 m deep. They are completely (Cockatoo) or partially (Molar) rimmed by profuse living coral and surrounded by lagoonal depths of 5-10 m. The inner slopes of the Cockatoo blue hole are 60-70° down to a depth of 25 m, below which coalescing sediment fans markedly reduce this angle. At the Molar blue hole, slopes are mainly gentler (45°) and sediment fans and terraces occur below 16 m. Distinct biological/sedimentary associations occur in both holes. Seismic refraction studies across the rim of the blue holes show a shallow (8.5-11 m) pre-Holocene surface beneath the rims. The balance of evidence suggests that the blue holes represent collapsed dolines which may have taken more than one low sea-level period to form. The original surface structures have been modified by subaerial solution processes, and subsequent sediment infill and coral growth following the Holocene transgression.

Lineage

Maintenance and Update Frequency: unknown
Statement: Unknown

Issued: 1979

This dataset is part of a larger collection

Click to explore relationships graph

152,-20.25 152,-21.75 150,-21.75 150,-20.25 152,-20.25

151,-21

text: westlimit=150.0; southlimit=-21.75; eastlimit=152.0; northlimit=-20.25

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