<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJG</journal-id><journal-title-group><journal-title>Open Journal of Geology</journal-title></journal-title-group><issn pub-type="epub">2161-7570</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojg.2015.54016</article-id><article-id pub-id-type="publisher-id">OJG-55454</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Facies Analysis and Depositional Environment of the Oligocene-Miocene Asmari Formation, Bandar Abbas Hinterland, Iran
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ahdi</surname><given-names>Hoseinzadeh</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Jahanbakhsh</surname><given-names>Daneshian</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Seyed</surname><given-names>Ali Moallemi</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ali</surname><given-names>Solgi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Geology, College of Basic Science, Tehran Science and Research Branch, Islamic Azad University, Tehran, Iran</addr-line></aff><aff id="aff2"><addr-line>Department of Geology, Faculty of Earth Science, Kharazmi University of Tehran, Tehran, Iran</addr-line></aff><aff id="aff3"><addr-line>Reservoir Geology Division, Exploration and Production Department, Research Institute of Petroleum Industry, Tehran, Iran</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>mhd_hoseinzadeh@yahoo.com(AH)</email>;<email>daneshian@khu.ac.ir(JD)</email>;<email>moallemisa@ripi.ir(SAM)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>04</month><year>2015</year></pub-date><volume>05</volume><issue>04</issue><fpage>175</fpage><lpage>187</lpage><history><date date-type="received"><day>3</day>	<month>February</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>6</month>	<year>April</year>	</date><date date-type="accepted"><day>9</day>	<month>April</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The Asmari Formation is a thick carbonate sequence of the Oligocene-Miocene in the Zagros Basin, southwest of Iran. This formation is located in Bandar Abbas and Coastal Fars regions on the following two sections: Anguro anticline (west-northwest of Bandar Abbas) and Gavbast anticline (southwest of Lar County). The Asmari Formation has diameters of 68 and 26 m in the Anguro and Gavbast sections, respectively. This formation is composed of limestone, dolomitic limestone and an altered form of marl. Based on the results of petrographic analyses, 7 facies were identified in the Anguro and Gavbast sections in the study region. The facies were deposited on the following 3 belts: tidal flat (MF 1 - 3), lagoon (MF 4 - 5) and open marine (MF 6, 7).
   
  According to evidence such as the gradual change of microfacies, the lack of main reef barriers, and the lack of slumping and sliding features, the Asmari Formation was formed in a marine environment of carbonate homoclinal ramp type. This environment is composed of the following two subenvironments: the inner ramp and the middle ramp. The comparison of the facies identified in the Anguro and Gavbast sections indicates that Gavbast section is mainly composed of lagoon facies. Moreover, the Anguro section demonstrates more facies diversity than Gavbast section.
 
</p></abstract><kwd-group><kwd>Asmari Formation</kwd><kwd> Depositional Environment</kwd><kwd> Microfacies</kwd><kwd> Ramp</kwd><kwd> Bandar Abbas Hinterland</kwd><kwd> Iran</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The Asmari Formation (the most important reservoir of Iran) is a thick carbonate sequence of the Oligocene- Miocene in the Zagros Basin, southwest of Iran. The Asmari Formation at the type section consists of 314 m of limestone, dolomitic limestone and argillaceous limestone [<xref ref-type="bibr" rid="scirp.55454-ref1">1</xref>] . The Asmari Formation, at its type section, is deposited during the late Oligocene (Rupelian)-early Miocene (Burdigalian) (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The base of the Asmari Formation varies in age. For instance, toward the coastal Fars area, it is mainly Rupelian while in the Dezful Embayment, it ranges from Rupelian to Chattian [<xref ref-type="bibr" rid="scirp.55454-ref1">1</xref>] .</p><p>In spite of the extension of the deposits of the Asmari Formation in the Zagros Basin, these deposits have not been studied properly. In this research, numerous sections were studied for the careful examination of the Asmari Formation in the Bandar Abbas region, on the east of the coastal Fars (southwest of Lar County). Due to the lack of deposits associated with this formation in the majority of sections, the significance of this formation, and the limited spread of these deposits in the study area, the Anguro and Gavbast sections were selected (in spite of the low thickness of the Asmari Formation). The main objectives of this research were focused on 1) a description of the facies and their distribution on the Oligocene-Miocene carbonate platform, and 2) describing and interpreting the depositional environments represented by the Asmari Formation.</p></sec><sec id="s2"><title>2. Geological Setting</title><p>Based on the sedimentary sequence, magmatism, metamorphism, structural setting and intensity of deformation, the Iranian Plateau has been subdivided into eight continental fragments, including Zagros, Sanandaj-Syrjan, Urumieh-Dokhtar, Central Iran, Alborz, Kopeh-Dagh, Lut, and Makran [<xref ref-type="bibr" rid="scirp.55454-ref3">3</xref>] (<xref ref-type="fig" rid="fig2">Figure 2</xref>(a)). The Zagros Basin is composed of a thick sedimentary sequence that covers the Precambrian basement formed during the Pan-African</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Cenozoic stratigraphy of the Zagros Basin, after James and Wynd (1965) [<xref ref-type="bibr" rid="scirp.55454-ref2">2</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x6.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Location and Geological map of the study area. (a) General map of Iran showing eight geologic provinces, adapted from Lacombe et al. (2006) [<xref ref-type="bibr" rid="scirp.55454-ref17">17</xref>] and Mobasher and Babaie (2008) [<xref ref-type="bibr" rid="scirp.55454-ref18">18</xref>] ; (b) Sub-divisions of the Zagros Mountains and Fars Subbasin, after Motiei (1994) [<xref ref-type="bibr" rid="scirp.55454-ref1">1</xref>] , with situation of the study sections in Fars Province</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x7.png"/></fig><p>orogeny [<xref ref-type="bibr" rid="scirp.55454-ref4">4</xref>] . The total thickness of the sedimentary column deposited above the Neoproterozoic Hormuzsalt before the Neogene Zagros folding can reach over 8 - 10 km [<xref ref-type="bibr" rid="scirp.55454-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref6">6</xref>] . The Zagros Basin has evolved through a number of different tectonic settings since the end of Precambrian. The basin was part of the stable Gondwana supercontinent in the Paleozoic, a passive margin in the Mesozoic, and it became a convergent orogen in the Cenozoic [<xref ref-type="bibr" rid="scirp.55454-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref8">8</xref>] . During the Paleozoic, Iran, Turkey and the Arabian plate (which now has the Zagros Belt situated along its northeastern border) together with Afghanistan and India, made up the long, very wide and stable passive margin of Gondwana, which bordered the Paleo-Tethys Ocean to the north [<xref ref-type="bibr" rid="scirp.55454-ref9">9</xref>] . By the late Triassic, the Neo-Tethys Ocean had opened up between Arabia (which included the present Zagros region as its northeastern margin) and Iran, with two different sedimentary basins on both sides of the ocean [<xref ref-type="bibr" rid="scirp.55454-ref9">9</xref>] . The closure of the Neo-Tethys Basin, mostly during the late Cretaceous, was due to the convergence and northeast subduction of the Arabian Plate beneath the Iranian sub-plate [<xref ref-type="bibr" rid="scirp.55454-ref9">9</xref>] -[<xref ref-type="bibr" rid="scirp.55454-ref12">12</xref>] . The closure led to the emplacement of pieces of the Neo-Tethyan oceanic lithosphere (i.e., ophiolites) onto the northeastern margin of the Afro-Arabian plate (e.g., [<xref ref-type="bibr" rid="scirp.55454-ref13">13</xref>] -[<xref ref-type="bibr" rid="scirp.55454-ref15">15</xref>] ). Continent-continent collision starting in the Cenozoic has led to the formation of the Zagros Fold- Thrust Belt, continued shortening of the mountain range, and creation of the Zagros foreland basin. The late Cretaceous to Miocene rocks represent deposits of the foreland basin prior to the Zagros Orogeny, and subsequent incorporation into the colliding rock sequences. This sequence unconformably overlies Jurassic to Upper Cretaceous rocks. Compressional folding began during or soon after the deposition of the Oligocene-Miocene Asmari Formation [<xref ref-type="bibr" rid="scirp.55454-ref16">16</xref>] . On the basis of lateral facies variations, the Zagros Fold-Thrust Belt is divided into different tectonostratigraphic domains that from NW to SE are: the Lurestan Province or Western Zagros, the Izeh Zone and Dezful Embayment or Central Zagros, and ﬁnally Fars Province or Eastern Zagros [<xref ref-type="bibr" rid="scirp.55454-ref1">1</xref>] (<xref ref-type="fig" rid="fig2">Figure 2</xref>(b)).</p><p>Also, from southwest to northeast of the Zagros Basin the following zones are distinguished: Zagros folded belt, fold and thrust belt, High Zagros and crushed zone. The Zagros Basin is also one of the most proliﬁc oil reservoirs in the Middle East. The study area is located in the northeastern part of the Fars Interior Zone.</p></sec><sec id="s3"><title>3. Study Area and Methodology</title><p>Anguro section is situated on the Anguro anticline with a length of 45 km and a width of 12 km. It is located on the west-northwest of Bandar Abbas City. It has a latitude of 27˚16' and longitude of 55˚50'. Gavbast section is situated on the Gavbast anticline with a length of 30 km and width os 7 km. It is located on the southwest of Lar County (Fars Province). It has a latitude of 27˚14' and longitude of 53˚52'. In both of the sections under study, the lower boundary of the Asmari Formation is placed on the Jahrum Formation through a paraconformity. The upper boundary is conformable with the Gachsaran Formation (Figures 3(a)-(c)). Following field inspections, 70 samples were collected from the sections of interest to study the Asmari Formation.</p><p>Thin sections of the samples were also obtained for the purpose of microscopic studies. The resulting thin sections were stained using Dickson’s method [<xref ref-type="bibr" rid="scirp.55454-ref19">19</xref>] and alizarine red to spot the calcite and dolomite contents. In this study, the Dunham classification was used for the classification of carbonate rocks [<xref ref-type="bibr" rid="scirp.55454-ref20">20</xref>] . Facies were also classified based on Fugel’s standard facies [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] and sedimentary environments were described based on Buxton and Pedley classification [<xref ref-type="bibr" rid="scirp.55454-ref22">22</xref>] .</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Field photographs showing: (a) A west view of the Anguro Section (lower boundary of the Asmari Formation with Jahrum Formation); (b) Upper boundary of the Asmari Formation with Gachsaran Formation is identified with paleosoil horizon in Anguro Section; (c) A east view of the Gavbast Section (Lower boundary and upper boundary of the Asmari Formation with Jahrum Formation and Gachsaran Formation respectively)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x8.png"/></fig></sec><sec id="s4"><title>4. Previous Works</title><p>Interest in the study of the paleontology, stratigraphy, and sedimentary environment of the Asmari Formation has been largely motivated by the exploration for oil and gas, because it contains more than 90% of Iran’s oil. The Asmari Formation was adopted after the Asmari anticline located in the northern Dezful Embayment and was referred to a sequence of Cretaceouse-Eocene in age [<xref ref-type="bibr" rid="scirp.55454-ref23">23</xref>] . The Asmari Formation was measured and deﬁned as an Oligocene nummulitic limestone by Richardson [<xref ref-type="bibr" rid="scirp.55454-ref24">24</xref>] and described by Thomas [<xref ref-type="bibr" rid="scirp.55454-ref25">25</xref>] as an Oligocene-Mi- ocene carbonate interval. James and Wynd [<xref ref-type="bibr" rid="scirp.55454-ref2">2</xref>] summarized previous viewpoints and ﬁnally formally deﬁned the Asmari Formation. Recently, the studies of biostratigraphy, depositional environment and sequence stratigraphy have been undertaken by Seyraﬁan et al. [<xref ref-type="bibr" rid="scirp.55454-ref26">26</xref>] , Seyraﬁan [<xref ref-type="bibr" rid="scirp.55454-ref27">27</xref>] , Seyraﬁan and Mojikhalifeh [<xref ref-type="bibr" rid="scirp.55454-ref28">28</xref>] , Vaziri-Mog- haddam et al. [<xref ref-type="bibr" rid="scirp.55454-ref29">29</xref>] , Amirshahkarami et al. [<xref ref-type="bibr" rid="scirp.55454-ref30">30</xref>] and Hakimzadeh and Seyraﬁan [<xref ref-type="bibr" rid="scirp.55454-ref31">31</xref>] . Ehrenberg et al. [<xref ref-type="bibr" rid="scirp.55454-ref32">32</xref>] and Laursen et al. [<xref ref-type="bibr" rid="scirp.55454-ref33">33</xref>] examined the Asmari Formation based on Sr isotope stratigraphyand revised age ranges mostly for the lower and middle parts of the Asmari Formation. Moreover, salinity changes duringthe late Oligocene to early Miocene for deposition of the Asmari Formation have been described by Mossadegh et al. [<xref ref-type="bibr" rid="scirp.55454-ref34">34</xref>] .</p></sec><sec id="s5"><title>5. Lithology</title><p>According to the results of field examinations of the study area, the thickness of the Asmari Formation increases relatively from the north to the south in the Bandar Abbas region. Therefore, the thickness of this formation in the Anguro and Gavbast anticlines is approximately 68 and 26 m, respectively. A total of 59 samples were obtained from the deposits of the Asmari Formation which were located in the Anguro section with a thickness of 68 m. This formation forms the heights and resistant areas due to its limestone lithology and high resistance to erosive factors. The lower boundary of the Asmari Formation is placed on top of shallow limestones of the upper part of the Jahrum Formation through a paraconformity (as a result of the absence of assemblage zone no. 58). The Asmari Formation contained within the Anguro section includes sequences of limestone, dolomitic limestone, and an alternation of marl and gray limestone. At the base of the Asmari Formation located on this section, gray limestones enriched with large benthic foraminifera accumulations (such as Nummulites intermedius-fichteli) were found next to other skeletal components (such as bivalves and echinoid debris) (<xref ref-type="fig" rid="fig4">Figure 4</xref>).</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Faunal distribution, biozonation and lithology of the Asmari Formation at Anguroan Gavbast sections</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x9.png"/></fig><p>The upper parts of the Asmari Formation contain sequences of thick dolomitic limestone and an alternation of limestone and marl. Large benthic foraminifera and bivalve fossils are also abundant in this section. There are also numerous fractures in this formation. The upper boundary of the Asmari Formation is conformable with the Gachsaran Formation. The evaporative Gachsaran Formation contains sequences of evaporate rocks located on the limestones of the Asmari Formation. The Gachsaran Formation demonstrates a milder topography as compared to the heights and walls formed by the Asmari Formation. That part of the Asmari Formation which is located on the Gavbast section has a total thickness of 26 m (<xref ref-type="fig" rid="fig4">Figure 4</xref>). This formation in this section was fully examined and 11 samples were obtained from it. Paleontological studies suggest that the lower boundary of the Asmari Formation is placed on the shallow limestones of the upper section of the Jahrum Formation. The part of the formation that lies on this section includes sequences of gray limestone. At the base of the section, the Asmari Formation includes gray limestone enriched with large benthic foraminifera accumulations (such as Archaias operculiniformis) and skeletal components (such as bivalves and echinoid debris). The upper parts of the formation embrace sequences of thick limestone as well as plenty of large benthic foraminifera and bivalve fossils. In the study area, the Gachsaran Formation lies on the Asmari Formation with in the conformable. It also demonstrates a milder topography as compared to the heights and walls formed by the Asmari Formation.</p></sec><sec id="s6"><title>6. Biostratigraphy</title><p>Biostratigraphic criteria of the Asmari Formation were established by Wynd [<xref ref-type="bibr" rid="scirp.55454-ref35">35</xref>] (<xref ref-type="table" rid="table1">Table 1</xref>) and reviewed by Adams and Bourgeois [<xref ref-type="bibr" rid="scirp.55454-ref36">36</xref>] (<xref ref-type="table" rid="table2">Table 2</xref>) in unpublished reports only. Based on the foraminiferal assemblages, the Asmari Formation is divided into lower, middle, and upper units. From base to top, three foraminiferal assemblages were recognized in the study area:</p><p>1) Assemblage l is characterized by the presence of Rotalia viennotti, Ditrupa sp., Planorbulina sp., Spirolina cylindracea, Austrotrillina asmariensis, Paragloborotalia spp. and coral and echinoid debris. This microfauna correspond to the Nummulites intermedius-Nummulites vascus Assemblage zone of Wynd [<xref ref-type="bibr" rid="scirp.55454-ref35">35</xref>] and Eulepidina-</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Biozonation of the Asmari Formation, Wynd (1965)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Formation</th><th align="center" valign="middle" >Biozone</th><th align="center" valign="middle" >Age</th></tr></thead><tr><td align="center" valign="middle" >Basal limestones of the Asmari Formation</td><td align="center" valign="middle" >56. Lepidocyclina-Opercolina-Ditropaassemblage zone</td><td align="center" valign="middle" >Oligocene?</td></tr><tr><td align="center" valign="middle" >Lower Part of Asmari Formation</td><td align="center" valign="middle" >57. Nummulites intermedius-Nummulites vascus assemblage zone</td><td align="center" valign="middle" >Oligocene</td></tr><tr><td align="center" valign="middle" >Lower Part of Asmari Formation</td><td align="center" valign="middle" >58. Archaias operculiniformis totalrange zone Oligocene</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Middle Part of Asmari Formation ―Lowest Levels of the Gachsaran Formation</td><td align="center" valign="middle" >59. Austrotrillina howchini-Peneroplis evolutus assemblage zone 60. Austrotrillina howchini-Peneroplis evolutus (Gachsaran Fm.)</td><td align="center" valign="middle" >Lower Miocene (Aquitanian)</td></tr><tr><td align="center" valign="middle" >Upper Part of Asmari Formation―Lower Parts of the Gachsaran and Razak Formations</td><td align="center" valign="middle" >61, 62. Borelis melo curdica zone</td><td align="center" valign="middle" >Lower Miocene (Burdigalian)</td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Biozonation of the Asmari Formation, (Adams and Bourgeois, 1967)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Formation</th><th align="center" valign="middle" >Biozone</th><th align="center" valign="middle" >Age</th></tr></thead><tr><td align="center" valign="middle" >Upper Part of Asmari Formation</td><td align="center" valign="middle" >1. Borelis melo group―Meandropsin iranica Assemblage Zone</td><td align="center" valign="middle" >Early Miocene (Burdigalian)</td></tr><tr><td align="center" valign="middle" >Middle Part of Asmari Formation</td><td align="center" valign="middle" >2. Miogypsinoides-Archaias-Valvulina Zone 2a. Elphidium sp. 14―Miogypsina Assemblage Subzone 2b. Archaias Asmaricus-Archaias hensoni Assemblage Subzone</td><td align="center" valign="middle" >Early Miocene (Aquitanian)</td></tr><tr><td align="center" valign="middle" >Lower Part of Asmari Formation</td><td align="center" valign="middle" >3. Eulipidina-Nephrolepidina-Nummulites Assemblage zone</td><td align="center" valign="middle" >Oligocene</td></tr><tr><td align="center" valign="middle" >Base of the Asmari Formation</td><td align="center" valign="middle" >4. Globigerina spp. Assemblage Zone (Wynd, 1965)</td><td align="center" valign="middle" >Oligocene</td></tr><tr><td align="center" valign="middle" >Jahrom Formation</td><td align="center" valign="middle" >5. Nummulites spp. Discocyclina spp. Assemblage Zone</td><td align="center" valign="middle" >Late Eocene (Probably)</td></tr><tr><td align="center" valign="middle" >Jahrom Formation</td><td align="center" valign="middle" >6. Coskinolina-Rhapydionina Assemblage Zone</td><td align="center" valign="middle" >Middle Eocene (Probably)</td></tr></tbody></table></table-wrap><p>Nephrolepidina-Nummulites Assemblage Zone of Adams and Bourgeois [<xref ref-type="bibr" rid="scirp.55454-ref36">36</xref>] . The faunal assemblage of this zone suggests a Rupelian-Chattian age.</p><p>2) Assemblage ll is characterized by the presence of Paragloborotalia spp., Pyrgo spp., Triloculina sp., Russella spp., Quinqueloculina spp., Praerhapydionina delicata, Textularia spp., Elphidium spp., Valvulina spp., Penarchaias glynnjonesi, Triloculina tricarinata, Austrotrillina asmariensis, Austrotrillina sp., Schlum bergerina sp. Archaias operculiniformis, Archaias sp., Peneroplis thomasi, Peneroplis evolutus, Peneroplis sp., Spirolina spp., Dendritina rangi. This microfauna correspond to the Archaias operculiniformis total range zone of Wynd [<xref ref-type="bibr" rid="scirp.55454-ref35">35</xref>] and Eulepidina-Nephrolepidina-Nummulites Assemblage Zone of Adams and Bourgeois [<xref ref-type="bibr" rid="scirp.55454-ref36">36</xref>] . The faunal assemblage of this zone suggests a Chattian age.</p><p>3) Assemblage lll is characterized by the presence of Dendritina rangi, Spirolina sp., Peneroplis sp., Archaias sp., Discorbis sp., Miliolids, Globorotalia spp. and Asterigerina rotula. This microfauna correspond to the Austro- trillina howchini-Peneroplis evolutus assemblage zone of Wynd [<xref ref-type="bibr" rid="scirp.55454-ref35">35</xref>] and Miogypsinoides-Archaias-Valvulinid Assemblage Zone of Adams and Bourgeois [<xref ref-type="bibr" rid="scirp.55454-ref36">36</xref>] . The faunal assemblage of this zone suggests a Aquitanian age.</p></sec><sec id="s7"><title>7. Facies Description and Depositional Environment</title><p>Seven carbonate sedimentary facies were recognized for the Asmari Formation in the study area. These facies are related to three depositional settings (tidal ﬂat, lagoon and open marine) of inner and middle portions of a carbonate platform.</p><sec id="s7_1"><title>7.1. Tidal Flat Facies Association</title>MF 1: Dolo Mudstone<p>This microfacies has been observed in the upper part of the Asmari Formation. The MF 1 consists of dolomicrite with fine dolomite crystals 5 to 16 &#181;m (<xref ref-type="fig" rid="fig5">Figure 5</xref>(a)). Bioturbation is also common (<xref ref-type="fig" rid="fig5">Figure 5</xref>(b)). There is no</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Photomicrographs showing: (a) Dolomudstone (XPL); (b) Bioturbation; (c) Silt-sized quartz grain scattered in matrix (XPL); (d) Dolo intraclast wackestone with silt-sized quartz grains; (e) Dolo peloid intraclast wackestone with silt-sized quartz grains (XPL); (f) Bioturbation (XPL); (g) Aggradational neomorphism in dolomicrite forming dolomicrosparite; (h) Ooid packstone to grainstone (PPL); (i) Milliolides as a core of a surficial ooid (PPL)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x10.png"/></fig><p>bioclast in this microfacies. Silt-sized quartz grains are scattered in the dolomicrite matrix (&lt;10%) (<xref ref-type="fig" rid="fig5">Figure 5</xref>(c)). Based on the presence of dolomicrite, detrital quartz grains, bioturbation, and the lack of bioclasts and comparison to the standard microfacies of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] , it can be concluded that microfacies MF 1 has been deposited in supratidal to upper intertidal environment. This microfacies is equivalent to RMF 22 of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] and Facies Belt 1 of Buxton &amp; Pedley’sclassification [<xref ref-type="bibr" rid="scirp.55454-ref22">22</xref>] .</p></sec><sec id="s7_2"><title>7.2. MF 2: Bioclast/Pelloid/Intraclast Wackestone</title><p>This microfacies consists of a wackestone with intraclasts (10%), peloid (7%) and bioclasts (Miliolides) (5%). Silt-sized grains of quartz are scattered in the matrix (<xref ref-type="fig" rid="fig5">Figure 5</xref>(d) and <xref ref-type="fig" rid="fig5">Figure 5</xref>(e)). This microfacies is mostly dolomitized. Bioturbation (<xref ref-type="fig" rid="fig5">Figure 5</xref>(f)) and neomorphism is the common diagenetic processes observed. Aggradational neomorphism of dolomicrite to dolomicro sparite is also common (<xref ref-type="fig" rid="fig5">Figure 5</xref>(g)). Based on the presence of carbonate mud, detrital quartz grains, bioturbation, and vertical relationship with tidal flat facies, and comparison to standard microfacies of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] , it can be concluded that the MF 2 has been deposited in the lower part of intertidal environment. Presence of intraclasts indicates high energy conditions. This microfacies is equivalent to the RMF-24 of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] .</p></sec><sec id="s7_3"><title>7.3. MF 3: Ooid Packstone to Grainstone</title><p>The texture of this microfacies varies from packstone to grainstone, and Ooid is the main allochem of this microfacies. Skeletal debris are Miliolides. Benthic foraminifera like Peneroplis sp., Peneroplis evolutus archaias sp., Austrotrillina howchini and bivalve debris are present. Superficial and two layer Ooids are well sorted. Lagoonal bioclasts formed the core of the Ooids (<xref ref-type="fig" rid="fig5">Figure 5</xref>(h) and <xref ref-type="fig" rid="fig5">Figure 5</xref>(i)). The presence of well-sorted, superficial, fine grained (&gt;0.5 mm) Ooids, lagoonal fauna as Ooid cores, the presence of grain-supported texture, and the vertical change of this microfacies to a tidal flat microfacies (MF 1 and MF 2) indicate deposition of MF 3 in a tidal channel environment with medium to high energy condition [<xref ref-type="bibr" rid="scirp.55454-ref37">37</xref>] .</p></sec><sec id="s7_4"><title>7.4. Lagoon Facies Association</title>MF 4: Bioclast Wackestone to Packstone<p>The MF 4 microfaciesis characterized by a wackestone to packstone texture. The amount of allochems varies from 30% to 50%. The main allochems of this microfacies are bioclasts (<xref ref-type="fig" rid="fig6">Figure 6</xref>(a)). Different types of bioclasts including: Quinqueloculina spp., Pyrgo spp., Triloculina tricarinata, Spirolina spp., Triloculina sp., Peneroplis evolutus, Peneroplis thomasi, Peneroplis planatus, Austrotrillina paucialveolata, Dendritina rangi (small benthic foraminifera), Lithophyllum sp., Lithothamnium sp., Lithoporella sp. (Red Algae), coral debris, Ditrupa sp., echinoid debris, bivalve debris, ostracod shells, Textularia spp., Russella spp., Asterigerina rotula, Elphidium sp.1, Ammonia beccari, Austrotrillina sp., Archaias sp., Peneroplis sp., Spirolina cylindracea, Austrotrillina asmariensis, Archaias kirkukensis (large benthic foraminifera) are present in this microfacies. Peloid is a subordinate nonskeletal allochems. Bioturbation (<xref ref-type="fig" rid="fig6">Figure 6</xref>(b)) and dolomitization are diagenetic processes which affected this microfacies. Dolomitization may be assumed fabric-selective as shown by the micritic matrix that was dolomitized while the allochems remained calcareous (<xref ref-type="fig" rid="fig6">Figure 6</xref>(c)). Textural characteristics, abundant porcelanaceous foraminifera (such as Miliolids), red algae, and benthic foraminifera, peloids, the presence of lime mud and bioturbation indicates high-energy lagoon near tidal flat [<xref ref-type="bibr" rid="scirp.55454-ref29">29</xref>] . Mixing of porcelanaceous foraminifera with open marine fauna like echinoids and reworked Nummulites (hyaline test) indicates that these sediments have been deposited in a lagoon attached to open marine waters by a tidal channel. This microfacies is equivalent to the RMF-20 of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] and facies belt 2 of Buxton &amp; Pedley [<xref ref-type="bibr" rid="scirp.55454-ref22">22</xref>] . Shallow depth and medium to low energy and presence in the photic zone is the characteristic of this environment. Some porcelanaceous perforate foraminifera (Peneroplis and Archaias) live in recent tropical and subtropical shallow water environment [<xref ref-type="bibr" rid="scirp.55454-ref38">38</xref>] .</p></sec><sec id="s7_5"><title>7.5. MF 5: Benthic Foraminifera Pelloidal Packstone to Grainstone</title><p>This microfacies is grain-supported with the texture of packstone (<xref ref-type="fig" rid="fig6">Figure 6</xref>(d)) to grainstone (<xref ref-type="fig" rid="fig6">Figure 6</xref>(e)). It consists of abundant porcelanaceous foraminifera like Triloculina trigonula, Spiroloculina spp., Pyrgo spp., Russella spp., Spirolina spp., Bigenerina sp., Triloculina sp., Triloculina tricarinata, Archaias operculiniformis, Elphidium sp.1, Ammonia beccari, Austrotrillina paucialveolata, Austrotrillina sp., Archaias sp., Peneroplis sp.,</p><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Photomicrographs showing: (a) Bioclast wackestone with lagoonal benthic foraminifera. Nummulites are also available (PPL); (b) Dolomitization. The matrix is dolomitized while allochems remains calcareous (PPL); (c) Bioturbatoin (PPL); (d) Benthic foraminifer pelloidal packstone (PPL); (e) Benthic foraminifer pelloidal grainstone. (PPL); (f) Bioclast echinoid packstone (PPL); (g) Bioclast coral rudstone (PPL); (h) and (i) Nummulites bioclast packstone (PPL)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x11.png"/></fig><p>Peneroplis planatus, Peneroplis evolutus, Peneroplis thomasi, Rotalia viennotti, Meandropsina iranica, Archaias kirkukensis, and non-foraminifera fossils like red algae (Lithophyllum sp. and Lithoporella sp.), bryozoans (Tubucellaria spp.), echinoids, trace fossils (Faverina asamarica), and peloids (<xref ref-type="fig" rid="fig6">Figure 6</xref>(e)). The amount of allochems ranges between 40% to 60%. Bioturbation, micritization (<xref ref-type="fig" rid="fig6">Figure 6</xref>(e)) and dolomitization are the main diagenetic features of this microfacies. Isopachous rim cement is present in grainstone texture. The presence of benthic foraminifera with porcelanaceous test, peloid, bioturbation and micritization indicates that the microfacieshas been deposited in the lagoon [<xref ref-type="bibr" rid="scirp.55454-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref40">40</xref>] . The faunal association characterizes an inner part of the platform [<xref ref-type="bibr" rid="scirp.55454-ref41">41</xref>] . The packstone to grainstone texture and presence of cement indicates deposition in shallow water depth above fair-weather Wave base, with medium to high energy conditions [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] , wide variety of fauna, the presence of stenohaline fauna (Echinoids and bivalve) and the mixing with porcelanous foraminifera indicate that this sediment have been deposited in an open lagoon environment with normal salinity. The MF 5 is equivalent to the RMF 20 and standard facies belt 2 [<xref ref-type="bibr" rid="scirp.55454-ref22">22</xref>] . The main characteristics of this environment are medium to low energy in the photic zone [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] .</p></sec><sec id="s7_6"><title>7.6. Open Marine Facies Association</title>MF 6: Bioclast (Coral) Echinoid Packstone to Rudstone<p>This microfacies is characterized by packstone to rudstone texture and consists of large fragments of fossils (&gt;2 mm) like corals, echinoids, bivalve, gastropods, and bryozoan especially (Tubucellaria spp.) (<xref ref-type="fig" rid="fig6">Figure 6</xref>(f) and <xref ref-type="fig" rid="fig6">Figure 6</xref>(g)). The amount of large fragments varies from 10% to 20%. Subordinate bioclasts with the amount 30% - 50% are present. Sorting is poor to medium. Syntaxial cement around echinoid debris are abundant.</p><p>The wide variety of marine fauna and microfauna (corals, echinoids, bivalve, and bryozoan (Tubucellaria spp.)) suggests deposition in open and oxygenate marine conditions, perhaps above the storm wave base (cf. [<xref ref-type="bibr" rid="scirp.55454-ref42">42</xref>] ). The MF 6 microfacies is equivalent to RMF-7 of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] and compares to the model of Buxton &amp; Padley [<xref ref-type="bibr" rid="scirp.55454-ref22">22</xref>] . It should be equivalent to facies belt 5, deposited in mid ramp environment.</p></sec><sec id="s7_7"><title>7.7. MF 7: Nummulite Bioclast Packstone</title><p>This grain-supported microfacies with packstone fabric mainly consists of bioclasts and Nummulites with the amounts of 30% to 50%. The main fossils present are Nummulites fichteli, Nummulites intermedius, Nummulites sp. and with a lower amount, Spirolina spp., Triloculina sp., Paragloborotalia spp., Peneroplis sp., Peneroplis planatus, Peneroplis evolutus, Peneroplis thomasi, Archaias kirkukensis and non-foraminifera are red algae including Lithophyllum sp., Lithothamnium sp., Lithoporella sp. However bioclasts of macro and microfossils debris including Ditrupa sp., echinoid debris, Faverina asmarica, bivalve debris, ostracod shells are also observed. Bioturbation is also common (<xref ref-type="fig" rid="fig6">Figure 6</xref>(h) and <xref ref-type="fig" rid="fig6">Figure 6</xref>(i)). Sorting is poor to medium.</p><p>The presence of hyaline test of microfauna like Nummulites and also stenohaline fauna such as echinoids, indicates deposition in a proximal open marine environment. Abundance and size of the Nummulites are good indicators of the depositional environments [<xref ref-type="bibr" rid="scirp.55454-ref43">43</xref>] . According to Racey [<xref ref-type="bibr" rid="scirp.55454-ref43">43</xref>] , elongate and large Nummulites have occurred offshore, in deeper water conditions with respect to other types of Nummulites, indicating increase in accommodation space. This microfacies is equivalent to the RMF-13 of Flugel [<xref ref-type="bibr" rid="scirp.55454-ref21">21</xref>] and facies belt 5 of Buxton &amp; Pedley [<xref ref-type="bibr" rid="scirp.55454-ref22">22</xref>] . The association of red algae and larger benthic foraminifera is known to inhabit the Oligo-photic zone of the middle ramp environment [<xref ref-type="bibr" rid="scirp.55454-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref41">41</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref45">45</xref>] .</p></sec></sec><sec id="s8"><title>8. Facies Association and Depositional Model</title><p>The results of the microfacies analysis indicate seven types of microfacies deposited in three standard facies belt: tidal flat (MF 1 - 3), Lagoon (MF 4, 5) and proximal open marine environment (MF 6, 7). A homoclinal ramp is proposed for the studied section composed of inner and mid-ramp, the inner ramp including tidal flat and lagoon subenvironments. This latter is indicated by the presence of dolomudstone, bioclast/peloid/intraclast wackestone to packstone, and ooid packstone/grainstone facies, while the lagoon by bioclast wackestone/packstone and benthic foraminifer peloidal packstone/grainstone (<xref ref-type="fig" rid="fig7">Figure 7</xref>).</p><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Schematic block diagram of depositional environment of the Asmari Formation in the Bandar Abbas area. Lateral distribution of microfacies in the sedimentary model, petrographic characteristics, and main carbonate particles of various facies are shown</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1210212x12.png"/></fig><p>The main components of these subenvironments are bioclasts of milliolids, Peneroplis sp., Peneroplis evolutus, Archaias sp., and Austrotrillina howchini, peloid, superficial Ooids, dolomicrite and detrital quartz. The mid ramp encompasses proximal open marine subenvironment as indicated by the bioclast (coral) echinoid packstone to rudstone, and Nummulite bioclast packstone facies.Main constituents include coral, bivalve, and gastropod debris, along with bryozoans, especially (Tubucellaria spp.). The presence of hyaline tests of microfauna like Nummulites as also stenohaline fauna, such as echinoids, indicates the deposition in a proximal open marine subenvironment (<xref ref-type="fig" rid="fig7">Figure 7</xref>). Previous studies considered different depositional platform types for the Asmari Formation. Some authors (e.g., [<xref ref-type="bibr" rid="scirp.55454-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref46">46</xref>] ) assumed the depositional environment of the Asmari Formation as shelf, while other workers (e.g., [<xref ref-type="bibr" rid="scirp.55454-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref30">30</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.55454-ref47">47</xref>] -[<xref ref-type="bibr" rid="scirp.55454-ref49">49</xref>] ) considered it as a carbonate ramp.</p><p>The results presented in the present report, based on the gradual changes of microfacies, the lack of main barrier reefs, and the slumping and sliding features, clearly suggest that the Asmari Formation has been deposited on a homoclinal ramp environment. Our results are in complete concordance with Pedley [<xref ref-type="bibr" rid="scirp.55454-ref50">50</xref>] who has proposed that during the Oligocene-Miocene, distally steepened and homoclinal ramps were widespread in Mediterranean areas.</p></sec><sec id="s9"><title>9. Conclusions</title><p>The thickness of the Asmari Formation increases from north to south in the Bandar Abbas area. In this area, this formation thickness is 68 and 26 m respectively in the Anguro and Gavbast sections.</p><p>The Asmari Formation in the Gavbast section has been deposited in an inner ramp. Fossil contents indicate that the lower contact of the Asmari Formation is with shallow marine carbonates of the Jahrum Formation. The upper contact of the Asmari Formation with the Gachsaran Formation is a disconformity.</p><p>The Asmari Formation contained within the Anguro section includes sequences of limestone, dolomitic limestone, and an alternation of marl and gray limestone.</p><p>In the Anguro and Gavbast sections, seven types of microfacies have been identified. These microfacies are interpreted as have been deposited in 3 microfacies belts, including tidal flat (MF 1 - 3), lagoon (MF 4, 5) and proximal open marine (MF 6, 7) environments. Gradual transition between microfacies, the lack of main barrier reef, and sliding and slumping features indicate the Asmari Formation has been deposited in a homoclinal ramp. Two subenvironments have been identified: inner ramp and mid-ramp. The lagoonal microfacies is the more abundant, followed by lagoon facies belt, the tidal flat (inner ramp) and proximal open marine facies belt are developed respectively.</p></sec><sec id="s10"><title>Acknowledgements</title><p>Research Institute of Petroleum Industry for permission for publication of this paper. The authors also appreciate Alireza Shakeri, Mehran Moradpour, Somayeh Parham, Mehdi Hadi, Rakhsahndeh Abbasi, Zahra Ahmadi, Morteza Fakhr Rahimiyan, Afshin Zohdi and Saeed Monibi for their cooperation during the project.</p></sec><sec id="s11"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.55454-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Motiei, H. (1994) Geology of Iran: Stratigraphy of Zagros. 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