The Cambrian Fossils of Chengjiang, China

The Flowering of Early Animal Life

Hou Xian-Guang, David J. Siveter, Derek J. Siveter, Richard J. Aldridge, Cong Pei-Yun, Sarah E. Gabbott, Ma Xiao-Ya, Mark A. Purnell, Mark Williams

• Publisher: Wiley-Blackwell
• Year: 2017
• ISBN:
  9781118896266
• Edition: 2
• Topic: Ciencias físicas
• Subtopic: Geología y ciencias de la Tierra

The celebrated lower Cambrian Chengjiang biota of Yunnan Province, China, represents one of the most significant ever paleontological discoveries. Deposits of ancient mudstone, about 520 million years old, have yielded a spectacular variety of exquisitely preserved fossils that record the early diversification of animal life. Since the discovery of the first specimens in 1984, many thousands of fossils have been collected, exceptionally preserving not just the shells and carapaces of the animals, but also their soft tissues in fine detail. This special preservation has produced fossils of rare beauty; they are also of outstanding scientific importance as sources of evidence about the origins of animal groups that have sustained global biodiversity to the present day.

Much of the scientific documentation of the Chengjiang biota is in Chinese, and the first edition of this book was the first in English to provide fossil enthusiasts with a comprehensive overview of the fauna. The second edition has been fully updated and includes a new chapter on other exceptionally preserved fossils of Cambrian age, exciting new fossil finds from Chengjiang, and a phylogenetic framework for the biota. Displaying some 250 figures of marvelous specimens, this book presents to professional and amateur paleontologists, and all those fascinated by evolutionary biology, the aesthetic and scientific quality of the Chengjiang fossils.

Part One
Geological and Evolutionary Setting of the Biota

1
Geological Time and the Evolution of Early Life on Earth

Our planet is some 4540 million years old. We have little record of Earth’s history for the first half billion years, but rocks have been found in Canada that date back some 4000 million years (Bowring & Williams 1999). There are yet older indications of the early Earth in the conglomerates of the Jack Hills of Australia, where tiny zircon crystals recycled from much older rocks give ages as old as 4400 million years (Wilde et al. 2001), and therefore their formation occurring a little after the birth of our planet. These zircons are important, because chemical signals within the crystals suggest the presence of water, a prerequisite for life on Earth, and also the lubricant for plate tectonics, which provides an active mineral and nutrient cycle to sustain life.

Because Earth’s history is so enormous from a human perspective, it has been divided up into more manageable packets of time, comprising four eons, the Hadean, the Archean, the Proterozoic, and the Phanerozoic (Fig. 1.1); the Hadean, Archean, and Proterozoic are jointly termed the Precambrian. In practice, the boundaries between these eons represent substantial changes in the Earth system driven by such components as plate tectonics, the interaction of life and the planet, and by the evolution of ever more complex biological entities. The boundary between the extremely ancient Hadean and Archean is set at about 4000 million years, whilst that between the Archean and Proterozoic is drawn at 2500 million years. The beginning of the Phanerozoic (literally meaning ‘manifest life’) is recognized by evolutionary changes shown by animals about 541 million years ago. The Archean is subdivided into the Eoarchaen (4000–3600 million years), the Paleoarchean (3600–3200 million years ago), the Mesoarchean (3200–2800 million years ago), and the Neoarchean (2800–2500 million years ago) eras. The Proterozoic is subdivided into the Paleoproterozoic (2500–1600 million years), the Mesoproterozoic (1600–1000 million years), and the Neoproterozoic eras (1000–541 million years). The earliest period of the Phanerozoic eon, the Cambrian, coined after the old Latin name for Wales, was a time that almost all of the major animal groups that we know on Earth today made their initial appearances in the fossil record. Some of the most important fossil evidence for these originations has come from the Chengjiang biota of southern China.

Figure 1.1 Some major events in the history of the Earth and early life.

However, the record of life on Earth goes back much further in time than the Cambrian Period, perhaps nearly as far as the record of the rocks. The early, Hadean Earth was subject to heavy bombardment by asteroids, many of which were so large that they would have vaporized early surface waters and oceans. This heavy bombardment ceased some 3900 million years ago, and from this period of the early Archean onwards there have been permanent oceans at the surface of planet Earth. Not long after – from a geological perspective – there is evidence for life. Microfossils of sulfur‐metabolizing bacteria are reported from Paleoarchean rocks as old as 3400 million years in Australia (Wacey et al. 2011), and there is circumstantial evidence from geochemical studies that carbon isotopes were being fractionated by organic processes as long ago as 3860 million years in the Eoarchean (Mojzsis et al. 1996). However, there is a need to treat some of the reports of evidence for very early life with caution, and the further back in time the record is extended the more controversial the claims become (see, e.g., Grosch & McLouglin 2014).

The sparse organic remains of the Archean are microscopic and sometimes filamentous. But there is also macroscopic evidence for early life, represented by microbial mat structures (Noffke et al. 2006) and stromatolites (Fig. 1.2). Modern stromatolitic structures are built up through successive layers of sediment being trapped by microbial mats. The resulting stromatolite forms are commonly dome‐like or columnar, and these characteristic shapes can be recognized in Paleoarchean sedimentary deposits up to 3500 million years old. Once again, the very oldest stromatolites are somewhat controversial, and it is possible that they could have been constructed by abiogenic processes rather than by living organisms (Grotzinger & Rothman 1996).

Figure 1.2 Representative fossils of the early history of life on Earth. (a) The trace fossil Treptichnus, burrows from early Cambrian strata in Sweden, signaling the movement of bilaterian animals through the seabed, ×1.5. (b) An Ediacaran acritarch, a probable resting cyst of a unicellular eukaryotic phytoplanktonic organism, ×1000; these were important primary producers in the Proterozoic and early Phanerozoic oceans. (c) Ediacaran organisms on a late Proterozoic marine bedding plane surface characteristic of Earth’s first widespread complex multicellular ecosystems; Mistaken Point, Mistaken Point Ecological Reserve, Newfoundland. The specimen upper center is about 20 cm long. (d) Late Proterozoic stromatolites, microbial mat structures; Bonahaven Formation, Islay, Scotland, see Estwing hammer for scale.

The microorganisms identified living in modern stromatolitic communities represent a wide range of types of life, including filamentous and coccoid cyanobacteria, microalgae, bacteria, and diatoms (Bauld et al. 1992). If we accept the combined evidence from microfossils, microbial mats, stromatolites and carbon isotopes, then it appears that life may have begun on Earth some 3500 million years ago, or possibly somewhat earlier, and that these life forms included microorganisms that could generate their own energy by chemo‐ or photosynthetic processes. Whether these earliest microorganisms used oxygenic photosynthesis – utilizing carbon dioxide and water to make energy and thereby releasing free oxygen – is controversial, and there is little evidence of a build‐up of oxygen in the Earth’s atmosphere until much later. But by the boundary between the Archean and Proterozoic eons, 2500 million years ago, cyanobacterial microorganisms using oxygenic photosynthesis had certainly evolved. These are responsible for one of the key events in the evolution of the Earth’s biosphere, the Great Oxygenation Event between 2400 and 2100 million years ago. This event led to atmospheric levels of oxygen rising to about 1% of the current level, and it is evidenced by the disappearance of reduced detrital minerals such as uraninite (uranium ore) from sedimentary deposits younger than this age worldwide (Pufahl & Hiatt 2012). The oxygenation of Earth’s atmosphere and hydrosphere was to have profound implications for the path of life. It provided new mechanisms of energy supply, and also pushed to the margins of existence in Earth’s earliest biosphere those organisms of the Archean that were adapted for an anoxic world and for which free oxygen was toxic.

There is a much richer and less controversial record of life in rock strata of Paleoproterozoic and Mesoproterozoic age. Microbial mats and stromatolites constructed by cyanobacteria are quite abundant, and it is likely that cyanobacteria had become diversified by the mid‐Paleoproterozoic (Knoll 1996). There are also fossil data showing that one of the most significant steps in evolutionary history had taken place by this time – the appearance of complex,...

Table of contents

• Cover
• Title Page
• Table of Contents
• Foreword
• Preface
• Part One: Geological and Evolutionary Setting of the Biota
• Part Two: Chengjiang Fossils
• References
• Systematic Index
• General Index
• End User License Agreement