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Tanner, Thomas; Hernández-Almeida, Iván; Drury, Anna Joy; Guitián, José; Stoll, Heather M (2020): New age points of ODP Hole 177-1088B [dataset]. PANGAEA, https://doi.org/10.1594/PANGAEA.924459, In: Tanner, T et al. (2020): New Tie points, organic and inorganic data, growth rate and pCO2 reconstructions for the late Miocene Cooling of ODP Hole 177-1088B [dataset bundled publication]. PANGAEA, https://doi.org/10.1594/PANGAEA.924529

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Abstract:
Composite core images for Ocean Drilling Program (ODP) Hole 1088B were generated by cutting individual core sections from core table photos (downloaded from JANUS: http://www-odp.tamu.edu/database/). Each section image was then compiled and scaled to the shipboard meters composite depth (mcd) using the Includes_Core_Table_Photos functions within Code for Ocean Drilling Data (CODD v1; www.codd-home.net; Wilkens et al. (2017)). To account for the single point lighting source used in core table photos, a lighting correction was also applied.
As shipboard color reflectance data was not collected at Site 1088, core color information (hue, saturation, lightness, red, green, blue) was extracted every mm from the composite core images using the CODD “CreateHoleCoreImageProfiles” function. The extracted lightness (L) showed the clearest variability and was chosen to approximate Lstar data. The top 4 cm of each section was excluded from the L profile to remove a lighting artefact at section ends. To account for core heterogeneity, the L data was then despiked using the CODD “Median_DeSpike” function (despiked data over 2 s.d. from the median within a 400 point/0.4 m window) and then smoothed using an 11-point binomial smoothing. All extracted data is provided in supplementary table 1.
The composite core images from Hole 1088B show clear evidence for core disturbance at the top of most cores (supplementary table 2). These intervals were excluded from the extracted lightness and shipboard magnetic susceptibility records. The shipboard magnetic susceptibility (MS) data was also despiked using the “Median_DeSpike” function (despiked data over 2 s.d. from the median within a 40 point/0.4 m window; supplementary tables 3).
An astrochronology for Hole 1088B was generated between 4.2 and 7.9Ma (38-90 mcd), using 24 minimal tie points between L maxima and ~110 kyr eccentricity maxima (Ecc; Laskar et al. (2004). These additional age points are provided in supplementary table 4.
Keyword(s):
Age model; ODP Site 1088B
Related to:
Tanner, Thomas; Hernández-Almeida, Iván; Drury, Anna Joy; Guitián, José; Stoll, Heather M (in review): Decreasing atmospheric CO2 during the Late Miocene Cooling.
Project(s):
Coverage:
Latitude: -41.136060 * Longitude: 13.562830
Date/Time Start: 1997-12-17T09:45:00 * Date/Time End: 1997-12-17T23:15:00
Minimum DEPTH, sediment/rock: 0.00 m * Maximum DEPTH, sediment/rock: 206.89 m
Event(s):
177-1088B * Latitude: -41.136060 * Longitude: 13.562830 * Date/Time Start: 1997-12-17T09:45:00 * Date/Time End: 1997-12-17T23:15:00 * Elevation: -2081.2 m * Penetration: 129 m * Recovery: 125.55 m * Location: South Atlantic Ocean * Campaign: Leg177 * Basis: Joides Resolution * Method/Device: Drilling/drill rig (DRILL) * Comment: 14 cores; 129 m cored; 0 m drilled; 97.3 % recovery
Parameter(s):
#NameShort NameUnitPrincipal InvestigatorMethod/DeviceComment
DEPTH, sediment/rockDepth sedmTanner, ThomasGeocode
AGEAgeka BPTanner, ThomasGeocode
Tie point typeTie point typeTanner, Thomas
Tie pointTie pointTanner, ThomasTieNum
Size:
84 data points

Data

Download dataset as tab-delimited text — use the following character encoding:


Depth sed [m]

Age [ka BP]

Tie point type

Tie point
0.000.000Core top0
1.370.126MiS 5e Hodell1
2.170.197MIS 72
4.120.407MIS 11 Hodell3
10.920.879MIS 20 Hodell4
20.731.950LO Discoaster brouweri5
22.602.390LO Discoaster pentaradiatus6
22.902.409MIS 96 Hodell7
23.382.490LO Discoaster surculus8
25.552.800LO Discoaster tamalis9
32.303.540LO Sphenolithus spp.10
33.653.700LO Reticulofenestra pseudoumbilicus11
38.794.173Prominent Lstar min to E min12
39.664.276Above core break (B5 to B6); Prominent Lstar min to E min - just after 2.4 Myr minimum13
45.645.003Lstar min to E min - just before 2.4 Myr minimum14
47.845.214Prominent Lstar min to E min15
48.855.290Small Lstar min to small E min16
50.625.484Lstar min to E min17
51.305.591Above core break; Lstar min to E min tie near LO D. quinqueramus (51.41 m to 5.59 Ma);18
52.785.742Directly above core break (B6 to B7); Lstar min to E min19
53.055.761Directly below core break (B6 to B7); Lstar min to E min20
55.135.859Lstar min to E min21
56.936.056Lstar min to E min22
60.586.250Above core break (B7 to B8); Lstar min to E min23
62.756.360Before core break (B7 to B8); Lstar min to Emin24
66.266.581Lstar max to E max25
67.276.674Lstar max to E max26
71.396.983Above core break (B8 to B9); Lstar min to E min27
72.937.119Below core break (B8 to B9); weak Lstar max to rough ET max near top Core 1088B-9H; in E minima - difficult to tie;28
74.507.211Lstar min to E(T) min; in E minima - difficult to tie;29
76.007.261Weak Lstar max to E max; in E minima - difficult to tie;30
79.947.436Above core break (B9 to B10); Weak Lstar max to almost E max near bottom Core 1088B-9H; in E minima - difficult to tie;31
82.747.580Below core break (B9 to B10); Lstar min to E min near top of Core 1088B-10H; in E minima - difficult to tie;32
84.997.684Lstar max to E(T) max; in E minima - difficult to tie;33
88.917.840Lstar min to E min - possibly a bit dubious as also near a core disturbance; in E minima - difficult to tie;34
90.097.940Lstar min to E min; Stopped below here due to cores overlapping etc.35
97.258.600FO Discoaster quinqueramus36
112.209.630LO Discoaster hamatus37
142.4910.470FO Discoaster hamatus38
169.8410.940LO Coccolithus miopelagicus39
206.8912.340FO Calcidiscus macintyrei40
206.8912.650LO Calcidiscus premacintyrei41