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Mitochondrial Eve

 
Who2 Biography: Mitochondrial Eve, Ancient Human

  • Born: 200000 B.C.
  • Birthplace: Africa
  • Died: c. 200,000 B.C.
  • Best Known As: Possibly the genetic 'mother' of all modern humans

A 1987 article in the journal Nature suggested the existence of a single ancient woman from whom all modern humans inherited mitochondrial genetic material. The primary author, Rebecca Cann, called this woman Eve and said she lived in Africa around the year 200,000 B.C. (Carr did not suggest that Mitochondrial Eve was the first human woman -- only that all later humans shared her genetic material.) The theory has been disputed by other scientists and continues to be explored.

The full title of the paper printed in Nature was "Mitochondrial DNA and Human Evolution"... Cann was a professor at the University of Hawaii; her co-authors on the paper were Berkeley's Allan Wilson and Mark Stoneking... Eve takes her name from the Bible's original woman, Eve... Another genetically interesting Eve was the alleged first human clone, 2002's Baby Eve.

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Science Dictionary: mitochondrial Eve
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When the original analysis of the DNA in the mitochondria of modern humans was carried out, the results suggested that all modern humans share the DNA of a single individual female who lived a few hundred thousand years ago. This female was named Eve in reference to the Creation story in the Book of Genesis in the Bible.

  • Further research has largely discredited the notion of a single Eve, although scientists have found that modern humans are descended from a very small population, perhaps as few as five thousand individuals.
  • Wikipedia: Mitochondrial Eve
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    Mitochondrial descendants of Eve

    Mitochondrial Eve (mt-mrca) is the name given by researchers to the woman who is defined as the matrilineal most recent common ancestor (MRCA) for all currently living humans. Passed down from mother to offspring, all mitochondrial DNA (mtDNA) in every living person is derived from hers. Mitochondrial Eve is the female counterpart of Y-chromosomal Adam, the patrilineal most recent common ancestor, although they lived at different times.

    Mitochondrial Eve is believed to have lived between 150,000 to 250,000 years BP, probably in East Africa, in the region of Tanzania and areas to the immediate south and west.[1] She lived during a period of time when Homo sapiens were developing as a species separate from other hominid species. She lived in a population of between perhaps 4000 to 5000 females capable of producing offspring at any given time. Mitochondrial Eve would have been roughly contemporary with humans whose fossils have been found in Ethiopia near the Omo River and at Hertho. Mitochondrial Eve lived significantly earlier than the out of Africa migration which might have occurred some 60,000 to 95,000 years ago.[2]

    Contents

    Matrilineal descent

    For more information on the principles involved, see matrilineal descent and genetic genealogy (matrilineal).

    To find the mitochondrial Eve of all living humans, one can start by tracing a line from every individual to his/her mother, then continue those lines from each of those mothers to their mothers and so on, effectively tracing a family tree backward in time based purely on mitochondrial lineages. Going back through time these mitochondrial lineages will converge on one maternal ancestor.

    This female, nick-named 'Eve', was of interest because she bore a mitochondrial genome (mitogenome) which was the template for all later human mitogenomes. Each human mitogenome bears mutations that have replaced some nucleotides on the Eve's mitogenome with other nucleotides (or in some cases added or removed nucleotides). These are called single nucleotide polymorphisms (SNPs). Mitogenomes are passed from mother to offspring, with very few exceptions—only rarely will the father's mitochondria persist long enough or in sufficient quantity to segregate to the germ cells. Consequently, recombination between paternal and maternal mitogenomes is not observed as with autosomal and X-chromosomal DNA. All complex animals can also trace their ancestry back to a mitochondrial MRCA. Chimpanzees and humans share a mitochondrial MRCA; further back in time, humans and gorillas share an earlier mitochondrial MRCA.

    Mitochondria within the cell have identical DNA sequence. On rare occasion, about once every 4,000 years a stable mutation occurs in a female that is passed to a female offspring and thus can be passed to subsequent generations.[3][note 1] At the time of the 'Eve' a mutation occurred that created either the proto-L0 or proto-L1 lineage, and began the two basal branches of human mitochondrial DNA, L0 and L1. However, this it can be inferred that Mitochondrial Eve had at least two daughters who survived to have their own children.[4] Because multiple mutations occurred on both lineages after mtDNA 'Eve' this new lineage cannot be determined.

    Estimating time to most recent common ancestor

    Estimated Coalescence time of human mitochondria MRCA (TMRCA) is a measure of genetic distance to predicted sequence of the human mitochondria most recent common ancestor. TMRCA is a product of coalescence analysis. There are two other major aspects: estimation of population size (and temporal structure) and estimating the place of coalescence, PMRCA. Of these coalescence analyses products, TMRCA is most important because population size estimates are heavily influenced by the TMRCA estimates. Two recent studies of human mitogenomes have produced current best estimates of the TMRCA of 194,300 and 192,000 years before present.[2][5] These estimates follow more than 30 years of research and the estimates continue to evolve. The process is described below.

    Coalescent ancestry of mtDNA

    Percentage of expected female offspring given number of total offspring
    # of
    offspring
    Number of females
    0♀ 1♀ 2♀ 3♀ 4♀
    0 100%
    1 50.0 50.0
    2 25.0 50.0 25
    3 12.5 37.5 37.5 12.5
    4 6.25 25.0 37.5 25.0 6.25

    Humans are sexually reproducing organisms composed of two dimorphic sexes. Individuals within mammalian species cannot create exact duplicates of themselves. Instead, each individual passes ~1/2 of their genetic makeup to offspring with their mate contributing the other half. Through offspring production, individuals increase their genetic representation in the next generation, increasing the probability that more of their genes will be passed.

    Mitochondria are overwhelmingly inherited from the female parent. Since female or male offspring are produced randomly at a ~1:1 ratios, when a mother passes a new mitochondrial mutation to her offspring there is random risk that the new mutation will be lost in the first generation. Alternatively the mutation may be passed to one or more female offspring and survive. If a mutation survives in a population long enough it may fix in that population (see figure:Most likely time in generations to fixation) as part of a forward looking process.[note 2][6]

    Most likely time in generations to fixation (N = 10)

    Estimating TMRCAs, however, requires the interpretation of a past process. The accumulation of SNPs creates new lineages and thus creates genetic diversity, whereas lineages are pruned by genetic drift. As scientist measure diversity they can estimate when lineages might have formed. The mutations that occurred along Eve's descendant lineages prevented her mitogenome from fixing; however the SNPs that accumulated on each lineage allow scientist to estimate the time in which she lived. Population genetic diversity is measured by pairwise genetic comparison or parsimony analysis. Felsenstein (2002) showed that parsimony analysis was preferential to pairwise distance analysis because it arranges the sequences into a tree, and thus it is possible to measure the distance from any mtDNA sequence to a predicted sequence of the MRCA. With a neutral assumption, the observation of a MRCA sequence that joins the two deepest branches at a single point infers a MRCA time (TMRCA). In addition to determining diversity mutation rate needs to be determined, and this is frequently referenced with external calibration.

    Calibrating the single nucleotide polymorphism rate

    There are two general methods of determining single nucleotide polymorphism (SNP) rates. The most precise method involves establishing a rate based on observing mutations in pedigrees (observing mutation rates between a very large number of parent-child pairs). The most practical and most frequently used method implements a phylogenetics approach; observing SNP rates between two deep branches in a population or between two species, such as between humans and chimpanzees. This second approach requires, generally, some form of paleontological anchor.

    In a recent review of mitochondrial clocking, Endicott et al. (2009) remarked that there is conspicuous disparity between rates estimated based on pedigrees and phylogenetics. Likewise, Soares et al. (2009) noted that the mutation rate is markedly higher than the observed SNP rate. One explanation for the disparity is that many deleterious mutations appear to be stable over a few generations but will be lost over large numbers of generations. Soares et al. (2009) suggest that these mutations can persist for 100s of thousands of years. Pedigree based rates would be more accurate for clocking recent migrations, and phylogenetic rates would be more accurate for estimate the time branch between two species when another similarly age branchpoint is already known. For estimating rates intermediate between short and long distance estimates Endicott et al. (2009) recommend using local or 'soft' calibration of the SNP rate (intra population based calibration) such as archaeologically defined colonization of different world regions.

    Studies that rely on the chimpanzee-human last common ancestor (CHLCA) are also proportionally affected by variance of the predicted TCHLCA from its actual age. Studies that rely on a pedigree based rate would not be capable of directly estimating events greater tha 50,000 accurately because substantial numbers of mutations would be lost due to purifying selection, and studies that rely on archaeological evidence may be troubled by classification issues and great paucity in the paleontological record. Therefore each method has one or more weaknesses.

    Estimating based on AMH archaeology

    Anatomical modern humans (AMH) spread out of africa and over very large intervals of geography and time left artifacts along the northern coast of the Southwest, South, Southast and East Asia Cann, Stoneking & Wilson (1987) did not rely on a predicted TCHLCA to estimate SNP rates. Instead they used evidence of colonization in Southeast Asia and Oceania to estimate mutation rates. Endicott et al. (2009) have reevaluated the predicted migrations globally and compared those to the actual evidence. They postulate that the molecular clock based on chimp-human comparisons is not reliable, particularly in predicting recent migrations, such as founding migrations into Europe, Australia, and the Americans. They have offered the recommendation that mitochondrial clocks for local branches that predict migrations should be calibrated based on local evidence of human occupation, and less reliant on the CHLCA. Endicott et al. (2009) tend to be most critical of the CHLCA when used to estimate local haplogroup evolution with less critique of the timing of mitochondrial Eve. It should be noted however that Cann et al. (1987) estimated the TMRCA of humans to be approximately 210 ky and the most recent estimates Soares et al. 2009 (using 7 million year chimpanzee human mtDNA MRCA) differ by only 9%, which is relatively close considering the wide confidence range for both estimates and calls for more ancient TCHLCA.

    Using RFLP technology

    This method has been used in a few but important early studies when sequence based methods were out of reach. Nucleotide sites in the mitogenome are variably functional. The optimum SNP rate selected depends largely on the sites selected for study. Based on this variation, there have been three general approaches that have been used with mitochondrial DNA to calculated the TMRCA: Restriction fragment length polymorphism (RFLP) analysis, hypervariable region (HVR; part of the D-loop that approximates the mitochondrial origin of replication, 1122 base-pairs) and coding sequence analysis. RFLP analysis has no direct assessment of rates, instead it internally calibrated the polymorphism rate based on archaeological evidence for 'founding' migrations to different continents.

    Using this method, Cann, Stoneking & Wilson (1987) estimated the sequence divergence rate between humans of different geographic origin at 2 to 4% per million years. Within Africa the highest sequence divergence, approximately 1.5% for D-loop, 0.25% for tDNA, 0.30% for rDNA and 0.4% for coding. Later studies would predict African sequence divergence in the D-loop to be between 2 and 5% which is higher than the 1.5% observed for the D-loop (see below). Within the non-D-loop one expects divergence of 0.1 to 0.3%, 0.08 to 0.25%, 0.16 to 0.45% for rDNA, tDNA and coding region, respectively. The RFLP values fall within the best estimate of the expected range as of 2009. The lower values for D-loop are the expected consequence of saturation as described in Soares et al. (2009). The anchoring method used by Cann et al. (2009), is based on c.1987 understanding of archaeology, which places humans in East Asia by 40 kya. However it is currently known that anatomically modern humans reached Southwestern China well before 42,000 years ago (ka). In addition, the dates of the Mungo Lake remains have been reestimated to between 42 and 63 Ka consistent with other recent evidence for earlier occupation. There is evidence of human occupation in India from 76 Ka, and the arguably anatomically modern human remains at Jebel Qafzeh have been reestimated to 93 ka. The underestimate of D-loop divergence rate resulted in an overestimate of the TMRCA while the underestimate of the age of human migration from Africa resulted in an underestimate, such that the errors largely balanced each other.

    Methods using time to CHLCA estimates

    Calibration methods
    one no longer has the option of considering a fossil older than about eight million years as a hominid no matter what it looks like.

    —V. Sarich, Background for man[7]

    Because chimps and humans share a matrilineal ancestor, establishing the geological age of that last ancestor allows the estimation of the mutation rate. However, fossils of the exact last common ancestor would be an extremely rare find. The chimp-human last common ancestor (CHLCA) is frequently cited as an anchor for mt-TMRCA determination because chimpanzees are the species most genetically similar to humans. However, there are no known fossils that represent that CHLCA, in fact there are no proto-chimpanzee fossils or proto-gorilla fossils that have been clearly identified.[note 3]

    In effect, there is now no a priori reason to presume that human-chimpanzee split times are especially recent, and the fossil evidence is now fully compatible with older chimpanzee-human divergence dates [7 to 10 Ma...

    —White et al. (2009), [8]

    Some researchers tried to estimate the age of the CHLCA (TCHLCA) using biopolymer structures which differ slight between closely related animals. Among these researchers, Allan C. Wilson and Vincent Sarich were pioneers in the development of the molecular clock for humans. Working on protein sequences they eventually determining that apes where closer to human than some paleontologist perceived based on the fossil record.[note 4] Later Vincent Sarich concluded that the TCHLCA was no greater than 8 million years in age, with a favored range between 4 and 6 million years before present.

    This paradigmatic age has stuck with molecular anthropology until the late 1990's, when others began questioning the certainty of the assumption. Currently, the estimation of the TCHLCA is less certain, and there is genetic as well as paleontological support for increasing TCHLCA. A 13 million year TCHLCA is one proposed age.[8][9]

    Despite having two known weaknesses,[10] the preferred method for determining the SNP rate is the phylogenetic based method calibrated by inter-species measurements. One weak point, the estimated TCHLCA is independent of the problems described above, and proportional variance of TCHLCA causes proportional errors of the TMRCA. The non-clocklike accumulation of SNPs, would tend to make more recent branches look older than they actually are. These two sources may balance each other or amplify each other depending on the direction of the TCHLCA error. There are two major reasons why this method is widely employed. First the pedigree based rates are inappropriate for estimates for very long periods of time. Second, while the archaeology anchored rates represent the intermediate range, archaeological evidence for human colonization often occurs well after colonization. For example, colonization of Eurasia from west to east is believed to have occurred along the Indian Ocean. However, the oldest archaeological sites that also demonstrate anatomically modern humans (AMH) are in China and Australia, greater that 42,000 years in age. However the oldest Indian site with AMH remains is from 34,000 years, and another site with AMH compatible archaeology is in excess of 76,000 years in age.[10] Therefore application of the anchor is a subjective interpretation of when humans were first present.

    SNP rates as described by Soares et al. (2009)
    Regions(s) Subregions
    (or site within codon)
    SNP rate
    (per site * year)
    Rate x TCHLCA Relative rate
    Control
    region
    HVR I 1.6 × 10−7 1.067 18.5
    HVR II 2.3 × 10−7 1.492 25.9
    remaining 1.5 × 10−8 0.100 1.74
    Protein-
    coding
    (1st and 2nd) 8.8 × 10−9 0.058 1.00
    (3rd) 1.9 × 10−8 0.125 2.17
    DNA encoding rRNA (rDNA) 8.2 × 10−9 0.053 0.92
    DNA encoding tRNA (tDNA) 6.9 × 10−9 0.045 0.78
    other 2.4 × 10−8 0.162 12.8
    TCHLCA assumed 6.5 Ma, relative rate to 1st & 2nd codons

    A simple measure the sequence divergence between humans and chimps by observing the SNPs. Given that the mitogenome is about 16553 base pairs in length (each base-pair which can be aligned with known references is called a site).[11] The formula is:

    rate = \frac{SNPs}{(2 T_{CHLCA}16553)}

    The '2' in the denominator is derived from the 2 lineages, human and chimpanzee, that split from the CHLCA. Ideally it represents the accumulation of mutations on both lineages but in different positions (SNPs). As long as the number of SNP observed approximates the number of mutations this formula works well. However, at rapidly evolving sites mutations are obscured by saturation affects. Sorting positions within the mitogenome by rate and compensating for saturation are alternative approaches. [12]

    Because the TCHLCA is subject to change with more paleontological information, the equation described above allows the comparison of TMRCA from different studies.

    Methods/parameters for estimating date of mitochondrial Eve
    Study Sequence
    type
    TCHLCA
    (sorting time)
    Referencing method
    (correction method)
    Cann, Stoneking & Wilson (1987) (RFLP) - archaeologically defined
    exo-African migrations
    Vigilant et al. (1991) HVR 4 to 6 Ma CH transversions,
    (15:1 transition:transversion)
    Ingman et al. (2000) genomic
    (not HVR)
    5 Ma CH genomic
    comparison
    Gonder et al. (2007) genomic
    (not HVR)
    6.0 Ma
    (+ 0.5 Ma)
    CH
    (rate class defined)
    Soares et al. (2009) genomic 6.5Ma
    (+ 0.5 Ma)
    CH, (3rd codons, certain HVR sites)
    Chimpanzee to Human = CH, LCA = last common ancestor
    Early, HVR, sequence based methods

    To overcome the affects of saturation, HVR analysis relied on the transversional distance between humans and chimpanzees.[13] A transition to transversion ratio was applied to this distance to estimate sequence divergence in the HVR between chimpanzees and humans, and divided by an assumed TCHLCA of 4 to 6 million years.[14] Based on 26.4 substitutions between chimpanzee and human and 15:1 ratio, the estimated 396 transitions over 610 base-pairs demonstrated sequence divergence of 69.2% (rate * TCHLCA of 0.369), producing divergence rates of roughly 11.5% to 17.3% per million years.

    HVR is exceptionally prone to saturation, leading to the underestimation of the SNP rate when comparing very distantly related lineages

    Vigilant et al. (1991) also estimated the sequence divergence rate for the sites in the rapidly evolving HVR I and HVR II regions. As noted in the table above, the rate of evolution is so high that site saturation occurs in direct chimpanzee and human comparisons. Consequently this study used transversions, which evolve at a slower rate than the more common transition polymorphisms. Comparing chimp and human mitogenomes, they noted 26.4 transversions within the HVR regions, however they made no correction for saturation. As more HVR sequence was obtained following this study, it was noted that the dinucleotide site CRS:16181-16182 experienced numerous transversions in parsimony analysis, many of these were considered to be sequencing errors. However the sequencing of Feldhofer I Neanderthal revealed that there was also a transversion between humans and Neanderthals at this site.[15] In addition, Soares et al. (2009) noted three sites in which recurrent transversions had occurred in human lineages, two of which are in HVR I, 16265 (12 occurrences) and 16318(8 occurrences).[note 5] Therefore, 26.4 transversions was an underestimate of the likely number of transversion events. The year 1991 study also used a transition-to-transversion ratio from the study of old world monkeys of 15:1.[citation needed] However, examination of chimp and gorilla HVR reveals a rate that is lower, and the examination of humans places the rate at 34:1.[3] Therefore this study underestimated that level of sequence divergence between chimpanzee and human. The estimated sequence divergence 0.738/site (includes transversions) is significantly lower than the ~2.5 per site suggested by Soares et al. (2009). These two errors would result in an overestimate of the human mitochondrial TMRCA. However, they failed to detect the basal L0 lineage in the analysis and also failed to detect recurrent transitions in many lineages, which also underestimate the TMRCA. Also, Vigilant et al (1991) used a a more recent CHLCA anchor of 4 to 6 million years.

    Coding region sequence based methods
    African mtDNA haplogroups
    L0

    L0d




    L0k




    L0f




    L0b



    L0a








    L1

    L1b



    L1c




    L5





    L2




    L6




    L3



    L4






    Partial coding region sequence originally supplemented HVR studies because complete coding region sequence was uncommon. There were suspicions that the HVR studies had missed major branches based on some earlier RFLP and coding region studies. Ingman et al. (2000) was the first study to compare genomic sequences for coalescence analysis. Coding region sequence discriminated M and N haplogroups and L0 and L1 macrohaplogroups. Because the genomic DNA sequencing resolved the two deepest branches it improved some aspects estimating TMRCA over HVR sequence alone. Excluding the D-loop and using a 5-million-year TCHLCA, Ingman et al. (2000) estimated the mutation rate to be 1.70 × 10−8 per site per year (rate * TCHLCA = 0.085, 15,435 sites).

    However, coding region DNA has come under question because coding sequences are either under purifying selection to maintain structure and function, or under regional selection to evolve new capacities.[16][17] The problem with mutations in the coding region has been described as such: mutations occurring in the coding region that are not lethal to the mitochondria can persist but are negatively selective to the host; over a few generations these will persist, but over thousands of generations these slowly are pruned from the population, leaving SNPs.[3] However, over thousands of generations regionally selective mutations may not be discriminated from these transient coding region mutations. The problem with rare mutations in the human mitogenomes is significant enough to prompt a half-dozen recent studies on the matter.

    Ingman et al. (2000) estimated the non-D loop region evolution 1.7 × 10−8 per year per site based on 53 non-identical genomic sequence overrepresenting Africa in a global sample. Despite this over-representation, the resolution of the L0 subbranches was lacking and one other deep L1 branches has been found. Despite these limitations that sampling was adequate for the hallmark study. Today, L0 is restricted to African populations, whereas L1 is the ancestral haplogroup of all non-Africans, as well as most Africans. Mitochondrial Eve's sequence can be approximated by comparing a sequence from L0 with a sequence from L1. By reconciling the mutations in L0 and L1. The mtDNA sequences of contemporary human populations will generally differ from Mitochondrial Eve's sequence by about 50 mutations.[2][18] Mutation rates were not classified according to site (other than excluding the HVR reigons). The TCHLCA used in the year 2000 study of 5 Ma was also lower than values used in the most recent studies.

    Inter-comparing rates and studies

    Molecular clocking of mitochondrial DNA has been criticized because of its inconsistent molecular clock.[19][20][21] A retrospective analysis of any pioneering process will reveal inadequacies. With mitochondrial the inadequacies are the argument from ignorance of rate variation and overconfidence concerning the TCHLCA of 5 Ma. Lack of historical perspective might explain the second issue, the problem of rate variation is something that could only be resolved by the massive study of mitochondria that followed. The number of HVR sequences that have accumulated from 1987 to 2000 increased by magnitudes. Soares et al. (2009) used 2196 mitogenomic sequences and uncovered 10,683 substitution events within these sequences. Eleven of 16560 sites in the mitogenome produced greater than 11% of all the substitutions with statistically significant rate variation within the 11 sites.[note 6] They argue that there is a neutral-site mutation rate which is a magnitude slower than rate observed for the fastest site, CRS 16519. Consequently, purifying selection aside, the rate of mutation itself varies between sites, with a few sites much more likely to undergo new mutations relative to others.[22] Soares et al. (2009) noted two spans of DNA, CRS 2651-2700 and 3028-3082, that had no SNPs within the 2196 mitogenomic sequences.

    The estimated time to mitochondrial Eve

    Early studies

    Allan Wilson and his colleagues began examining the mitochondrial molecular clock in the late 1970s and they found some regions of mitochondrial DNA evolve rapidly. Given sequencing technology of the time this was useful because many discrepant SNP could be detected over a short sequence of DNA.[23][24] In 1980, W.M. Brown, looking at the relative variation between human and other species, recognizes there was a constriction in the human population 180,000 years ago.[25] A year later Brown and Wilson were looking at RFLP fragments and determined the human population expanded more recently than other ape populations and noted that humans had the mtDNA diversity that was comparable to isolated subspecies of other apes.[26] The study described above by Cann, Stoneking & Wilson (1987) estimated the time in which mitochondrial Eve lived (human mitochondrial TMRCA) at 215 +/- 75 kya (142,500 and 285,000 years ago).

    Sequence based studies

    This was followed by Linda Vigilant's approach applifying the hypervariable region within the mitochondrial D-loop from the single hairs of southern African hunter-gatherers (!kung-San - a click speaking tribe of Namibia and neighboring Botswana).[27] At the time, it was believed that sequencing this region was advantageous because the larger density of mutations and because it was believed hypervariable region neutrality caused rapid SNP rate. Two years later, Vigilant et al. (1991) used the same technique and 4 to 6 million year TCHLCA range to produced human mtDNA TMRCA between 166,000 and 249,000 years. As described above the approach had a number of problems, indicating the need for a much larger TMRCA confidence interval in the study.

    TMRCA (in 1000 years; Ka) from different studies versus different TCHLCA
    Study Sequence
    divergence
    Assumed TCHLCA
    in million years
    Hdeepest CH 4 5 6.5 8 10 13
    Vigilant et al. (1991) 0.0287 0.692 166 Ka 207 270 332 415 539
    Ingman et al. (2000) 0.00582 0.17 137 171 223 274 343 446
    Gonder et al. (2007) not determined 120 149 194 239 299 389
    Soares et al. (2009) not determined 110 137 178 219 274 357
    Bolded values are published TMRCA for assummed TCHLCA, Vigilant et al (2009) is lower end of range. Soares et al. (2009) used at 6.5 Ma + 0.5 Ma sorting time.

    Advances in sequencing made it possible to sequence large numbers of genomic mitochondrial DNA (mitogenome). In 2000, Ingman et al. (2000) analyzing the non-HVR region of mitogenomes estimated mitogenomic TMRCA of 171,500 ± 50,000 years. This estimate was lower than previous studies, as this group continued to use a recent TCHLCA of 5 million years. However, the study did resolved the deepest branching of mitochondrial population in humans.

    Despite some agreement with this date in some anthropological circles, there was concern that this date was too recent. A growing body of evidence from the Levant (Skhul and Qafzeh), India, China and Australia (Mungo Lake- LM3) that humans had migrated from Africa well before 52 kya.[28] Higher-set TCHLCA places the upper limit of confidence above the age of the earliest non-Neanderthal hominids at Skhul. However, Tattersall and Schwartz (2008) recognize that some examples of late archaic homo sapiens in the Levant may be better placed in other (non-Homo [sapiens] sapiens) taxa as the Levant may not have been an early site of human occupation out of Africa.[29] Rightmire (2009) associates archaic humans from Jebel Irhoud (Morroco 160,000) in a Mousterian tool context with the early Skhul fossils and if this dating is correct (real date not less than the estimate) then it distances both Jebel Irhoud and the oldest Skhul fossils from the geographic limits of the constrict population. Because of the sample size this study failed to see evidence of selection or population size growth; however, coalescence theory predicts that under neutral models, current population size in Africa is far too great to explain coalescence as recent as 171,500 years ago without some selection.[30]

    The region in Africa where Tishkoff found the greatest level of mitochondrial diversity (green) and the region Behar et al. postulated the most ancient division in the human population began to occur (light brown)

    Gonder et al. (2007) undertook mitogenomic sequencing in areas of Africa were previous studies indicated deep diversity. This new study found new lineages of African mtDNA and more importantly narrowed the region within Africa in which humans ancestors likely arose. This new study indicated that the TMRCA likely occurred between 160,000 to 226,000 years ago (but dates between 130,000 and 280,000 cannot be ruled out, see TMRCA table).[2] This study was followed by Soares et al. (2009) which estimated the TMRCA at 192,000 years by singling out sites that were not as subject to purifying selection in the mitogenome.

    Estimated times of major mtDNA branchpoints

    The deepest branching lineage within the human mitochondrial population is the L0/L1 branches uncovered by Ingman et al. (2000). Beyond this, the L1 subbranches had largely been described by in the study of HVR regions in the decade previous to that study. The L0 subbranches have undergone intense study in the since 2000. Behar et al. (2008) examined the Khoisan population adding many more sequences. They determined that Khoisan mitogenomes other than the L0d and L0k appear to be the result of recent admixture. Consequently they estimated that Khoisans separated from the core interbreeding population after both the L0d and L0k clades had formed, about 144,000 years ago +/-11,000 years. In as much as their evidence suggested very low geneflow between non-Khoisan females and Khoisan females for 10,000s of years it was no longer possible for a population constriction to fix mtDNA in both groups, the period of constrained population size had effectively ended. Behar et al. (2008) derived their TMRCA from a 6.5 Ma TCHLCA which had a mutation frequency of 1 per 5182 years. This is about 80% the rate proposed by Soares but Soares used at larger TCHLCA therefore using Soares et al. methodology the branching of L0k would be about 125 ka.


    Superhaplogroup split times (in 1000 of years; Ka) from Soares et al. (2009) relative to different TCHLCA
    Split ("/")
    or node
    TCHLCA
    6 7 8 9 10
    L0k / L0a'f 118 Ka 138 158 178 197
    L1 / L2'5 143 167 191 215 238
    L2'3 / L5 127 148 170 191 212
    L2 / L3 98.3 115 131 148 164
    L3 61.4 71.6 81.8 92.1 103
    N 61 71.2 81.4 91.5 102
    M 51.9 60.6 69.3 77.9 86.6
    bolded values are given TCHLCA (+ sorting time) and split times from Table 3 and Figure 6 of Soares et al. (2009),

    Cann, Stoneking & Wilson (1987) used paleoanthropological evidence for human settlement in New Guinea, Australia and the New World allowing them to estimate the sequence divergence rate was 2 to 4% per million years(at the RFLP level). An ancestor "c" contained no known African ancestors and they suggest this ancestor lived between 90,000 and 180,000 years ago. Ingman et al. (2000) presented with an 'exodus' time from Africa in non-Africans of 52,000 years +/- 27,500 years (Assuming TCHLCA = 5 million years).[11]

    Genetic dating performed using rho [a measure of genetic distance] can be particularly distorted if the sequence data have not evolved with a constant population size through time; for example, due to the effects of founder effects, changes in effective population size, and bottlenecks, all features of human prehistory [Cox (2008),Nielson & Beaumont (2009)]. The performance of the rho statistics will be further compromised by the effects of natural selection, rate variation among sites, and rate variation among lineages.

    —Endicott et al. 2009

    Endicott et al. (2009) have recently reviewed the evidence for mutation rate variation and consider that the level of rate variation in humans, between lineages, is considerable. They have cast considerable critique on the use of global molecular clocks, but have particularly criticized the use of general molecular clocking on the timing of regional migrations. Therefore while considering that the TMRCA for mitochondrial Eve has tended to float around an estimated age of 200 Ka, more caution should be applied when considering the precise timing of migrations based on the MRCA of haplogroups, such as haplogroup M and N.

    Coalescent structure

    Population size estimates are one of the most important products of TMRCA determination. Based on the TMRCA and branching structure of the parsimony tree over time and geographic space these secondary products can be estimated:

    • The average population size throughout the from the TMRCA to present.
    • The complex structure of the population can be estimated.
    • Place of the MRCA (PMRCA).

    If population size is sufficiently large we might argue that Z was inclusive of all the similar morpho-metrically defined populations (i.e. fossil cousins) that existed at the time, but if Z is sufficiently small, one begin to look at the concept of speciation, the formation of a new species. In other words, the more that the boundaries of population size can be limited the more one is able to draw inferences about the population (its range, its location, its constituents).

    Summarizing, the rate at which a new allele will eventually will displace all deeper branching clades and the time that it takes is a probabilistic function of the population structure and ploidy based on forward looking statistics. Above, the complicities of calculating the TMRCA are discussed and the result of the process ls a broad range. Since populations size estimates are dependent on that range it will also occupy a large range.

    N = \frac{TMRCA}{2Tg} where Tg = generation time.

    As with the prediction of the TMRCA, variance of population size is a concern. If we assume a flat population structure then population size equals half the TMRCA in generations. Having a range of TMRCA then one need only determine the intergenerational distance (generation time) and the flatness of the structure. However depending on the branch (bushy versus stretched out). If the structure is fully stretched out with branches following a slowly increasing number over time, then one can predict the variance of population size similar to the method to establish variance about TMRCA estimates.

    Based on the early mtDNA studies and other early indirect studies Takahata estimated that the Ne, female was between 3,500 and 4,600 individuals.[31]

    Estimation of generation time

    Population sizes relative to Generation times and TMRCAs (see above)
    Generation
    time
    mtDNA TMRCA
    110,000 137,000 178,000 219,000 274,000 357,000
    20 years 2750 inds. 3425 4450 5475 6850 8925
    25 years 2200 2740 3560 4380 5480 7140
    TMRCA based on mutation rate estimates by Soares et al. (2009) and on TCHLCA of 4, 5, 6.5, 8, 10 and 13 Ma

    Early studies using mtDNA used generation time of 20 years based on numbers of studies of Neolithic peoples. However, it appears that population growth and higher densities of population after the Mesolithic has favored lower generation times. Studies from Europe's Mesolithic/Neolithic transition indicated that Mesolithic hunters typically were healthier and lived longer than their Neolithic counterparts. In addition, demographic studies of African hunter-gatherers revealed that peoples like the !kung have relatively long generation times, and as this group represents a major early branch within the human population then we must factor their reproductive behavior into estimation of generation times.

    Estimates of generation time now lie between 20 and 25 years, there appears to be a preference for 22 or 23 years.

    Estimating Eve's population size

    Estimates assuming a flat population structure

    If the population structure is assumed to be flat then the range of median estimated values has to be between 2200 and 9000 individuals, simply based on uncertainty about the mutation rate and generation times. The distribution of population sizes like TMRCA is an exponential function, and thus variance is also an exponential function, and with no other information one would create the crossproduct between the variance and TMRCAs to determine the appropriate population size distribution.

    Resolving more complex structure

    Retrograde look at bottlenecks. Diagram shows what genetic coalescence detects (grey area) in retrospective examination of the population, the alleles of more ancient TMRCA (circled in white) are not visible in the extant population, because they have been excluded prior to population expansion

    Population structure is heavily influenced by branching in several ways. An informative example is haplogroup M, after evolving in or entering Eurasia, the population expanded multifold.[32] Thus the number of M bearing lineages propagated, if this were not the case we would see several mutations between M and its 2 basal sublineages, but there are a dozen or so basal M lineages spread between Africa, South and East Asia. Another model that explains rapid growth of lineages would follow positive selection. Atkinson, Gray & Drummond (2009) argue that there were significant increases in the population size in mulitple lineages (L0, L1, L2 and especially L3) prior to 60 kya. Therefore many lineages could not be eliminated beyond 100,000 years ago with the population sizes that have existed in Africa for the last 100,000 years, and these lineages did not replace other lineages but grew in number as evidence for human expansion outward from Southeastern Africa. While these authors did not extrapolate backwards of 150,000 years (anchor = Ht Q in Papua New Guinea at 45 kya; with generation time of 20 years) and places the sum of lineage specific population sizes above 10,000 individuals before 100,000 years ago. They also demostrate a 95% confidence range before 150,000 years ago is between 1000 and 10,000 effective females. Because of the coalsence of lineages backward through time, population size cannot be extrapolated fertility backwards.

    Expansions are not required to prevent fixation events, isolation of groups can inhibit fixation. Within the Khoisan speakers of S. Africa, maternal lineages appear to have undergone 100,000 years of isolation.[18] Consequently, given that the World's population is magnitudes larger than the estimated size and that an inflection of size had to have occurred at some point, a good choice of points in which fixation became decreasingly possible lies between a temporal depth of 1/3 to 1/2 the retrospective time to the TMRCA. This means that the flatness of the population structure maybe restricted to Africa and at depths greater than 1/3 TMRCA. This effectively limits the maximum 'flat' shaped population during that period to less than 6000 effectively reproducing females (census of 18000 females).

    Solitary female Eve as a misconception

    Therefore increased knowledge of the branching structure better affords the estimation of population size. It should be noted that there is a model by which population could grow from very small numbers, a virtual 'Eve' if the population continues to expand at rate tolerant of preservation of the deepest branch. Using mtDNA alone cannot discriminate the 'early flat' model and a virtual 'Eve' model, however studies of other loci also point to a population size of about 10,000 effectively reproducing individuals, and extreme recent pinches in the population would result in abundant recent fixation of autosomal and X-linked loci. In contrast 90% of all X-link loci studies so far underwent fixation 100,000s of years before mtDNA TMRCA suggesting that population did not collapse to a single mating pair, and establishes a lower limit of the population size approximately 102 females, even for brief periods.[33] The concept of a solitary Eve within the human population is a misconception.[34][35][note 7]

    Selection on mitochondrial DNA sequence

    One of the most common measures implying structural changes are measures of selection. Selection in this context is not necessarily the same as positive selection in a competitive context. Fortuitous colonization of new territories by a small number of individuals can make unique alleles carried by those individuals appear selective to other individuals. If we apply this to humans, by creating a given in the argument that there was a place in Africa that was core to mtDNA of all humans and that there was at the geographic center of that core unique set of alleles. As the population expanded from the boundaries after the MRCA sequence had excluded all deeper branches then all the branches that expanded on the fringe would exhibit the appearance of positive selection relative to the allele that was unique to the central population. There are two measures of departure from Neutrality, the Tajima's D statistic and the D* and F* statistics of Fu and Li. As more mitogenomic sequence information has been gathered on Africa's hunter gatherers it appears there has been selection acting on Africa's basal lineages and that selection is not uniform.

    Implications

    The background for the interpretation of the mtDNA TMRCA are the numerous studies showing human-like fossils and bone remnants in Africa and Eurasia. These studies progress in concert with modern molecular genetics, with sequencing of ancient bone remnants becoming more common-place, particularly for Neandertals. Prior to the sequencing of the first Neandertal mtDNA, the TMRCA and PMRCA for modern humans set ancient humans apart from Neandertals. The current sequence of a number of Neanderthal mtDNA has reaffirmed that in the genus homo's recent past the female lineages of Neandertals and Humans existed in non-crossbreeding populations. Thus the implication of recent African origins 20 years ago set off one of the biggest battles in paleoanthropology, setting major players, such as Milford Wolpoff against molecular paleontologist such as AC Wilson.

    Mitochondrial 'Eve' appeared in the literature in 1987 supporting an 'Recent out of Africa' model that was a minority view at the time. The Multiregional evolution hypothesis (MREH) was the most popular at the time and continued to challenge the OoA model for more than a decade.

    Despite the compatibility of TMRCAs/PMRCAs from Neandertals and Humans with a multiple species model, other genetic studies ambiguously supported this theory. Y chromosomal studies produced a TMRCA, at less than 50,000 years, this estimate occurred after humans had expanded. Studies of other loci presented with a wide variety of fixation times, from 0 to 2 million years. Others studies did not adequately sample in Africa and presented ambiguous PMRCA or PMRCA on other continents.[36] Francisco Ayala tried to discredit the coalescent population size by arguing that the HLA-DRB1 locus had a TMRCA of 10s of millions of years.[37]

    Variance of neutral fixation times

    TMRCAs of loci, Y chromosome, and mitogenomes compared to their probability distributions if one assumes that population expanded 75kya from a long-standing population of 11,000 effective individuals

    One early oversight of many early studies is that the fixation of alleles (the object of coalescent theory study) is not a discrete mathematical function, it is a probabilistic function, and it is highly dependent on the ploidy being studied.

    Comparison to the X-linked and Autosomal TMRCAs

    Takahata (1999) was the first molecular anthropologist to point out that conclusions drawn from single locus studies suffer from the large randomness of the fixation process. Schaffner (2004) has cleared up this issue by demonstrating the 3 sets of fixation ranges, haploid, X-linked and diploid where TMCRAs for different loci are expected to fall. Takahata (1993) estimated the effective human population size at 11,000 individuals, and Schaffner working on an improved set of X-linked markers from low recombination regions of the X-chromosome identified an effective size of approximately 12,000 individuals.[38][39] PDHA1 falls on the edge of fixation times for X-linked chromosome. For autosomes, the MX1 locus and the HLA loci appear to preserve past diversity in the human population. With few exceptions, however, X-linked and autosomes appear to coalesce under a common population size.

    Comparison to the Y chromosomal TMRCA

    Just as mitochondria are inherited matrilineally, Y-chromosomes are inherited patrilineally.[40] Y chromosomal TMRCA, the time of the Y-chromosomal Adam, lie in the 42 to 110ky range, which is a little less than half the TMRCA of mtDNA. Importantly, the genetic evidence suggests that the most recent patriarch of all humanity is much more recent than the most recent matriarch, suggesting that 'Adam' and 'Eve' were not alive at the same time. While 'Eve' is believed to have lived more than 140,000 years ago, 'Adam' appears to have lived less than 110,000 years ago.[34] According to Wilder et al. (2004), the lower TMRCA of Y is due to an effective population size of males 1/2 that of females over most of human evolution.[41]

    Even with a reduced effective population size there are problems with this explanation . Recently, with more mitogenomic sequences from Africa, evidence has grown for an early population size expansion. This expansion probably started prior to 100,000 years ago and greatly increasing after 100,000 years ago(see: Population size oscillation). The effective size of the human population should have well exceeded 104 individuals between 80,000 to 120,000 years ago. Given this expansion, implicit male populations sizes would have improbably coalesced to Y-Adam within that time frame. However, the greatest age for Y TMRCA is more recent than the evidence for expansion. In addition, despite evidence of a bottleneck, the human mtDNA TMRCA range remains consistent with population sizes estimates from X-linked and autosomal loci. However, Y-chromosomes TMRCA is not consistent with mtDNA or either of these sets (see figure:TMRCAs of loci).

    This inconsistency maybe explained by some form of Y chromosome selection (cultural, or genetic). A Y-chromosomal lineage might have swept the male population.[42] However, if true the place of greatest Y chromosomal diversity could be anywhere that humans inhabited Africa. However, Y diversity is greatest in Southern Africa, close to the earliest female population split predicted by Behar et al. (2009) suggesting the earliest branch in Y should be between 125,000 and 150,000 Ka in age. This suggests a SNP rate inaccuracy in the Y-chromosomal and/or mtDNA molecular clock. A recent study of X-chromosome suggests that different rates of male sperm production between humans and chimps has altered the molecular clock in sex chromosomes.[43] This shift in the molecular clock would not affect the mtDNA SNP rate and would affect the Y-chromosomal rate more than X-linked and autosomes, since these Y-chromosomal lineages spend the most time in male testes.

    Population size oscillation

    The term bottleneck has been used to describe the population structure that created mtDNA Eve. The appearance of a bottleneck was a consequence of the appearance of a 'big bang' of HVR branching about the time humans first left Africa. From that point back to the TMRCA was less than 100,000 years and the population size estimate was below 5000 effective females. Looking backwards in time this is what might be called a retrograde bottleneck, however it is an artifact of coalescence process, since the coalescence of mitogenomes on the sequence of the MRCA (the event which initiated with mtDNA Eve and extended to the extant population) conceals the population size from all points earlier than that mutation (see figure Retrograde look at bottlenecks). Therefore the population size could have been of equal size going back 100,000s of years, to the time in which Neanderthals' ancestors and Modern humans' ancestors were part of a single population.

    Evidence against a population bottleneck

    The work done on Neanderthal sequencing (Green 2007) has identified little evidence of Neanderthal contribution to humans, moreover it describes an effective size of the population when humans and Neanderthals split was about 3000 individuals. Taken in the light of Schaffner's and Takahata's effective populations sizes, 3000 < Ne, female < 6000 and 2000 < Ne, male < 4000 does not appear to represent a magnitude shift downward from the average size. Taking a null hypothesis, prior to and after the mtDNA MRCA population sizes appear to reflect long-term small population structure up until 70,000~150,000 years ago, not a brief constricting bottleneck, but a long period of constrained size followed by an expansion.

    Evidence for a population bottleneck

    Confidence intervals of population size do not require an alternative, population bottleneck, hypothesis. However, a bottleneck may have existed. If the population size were at 12,000 individuals as suggested by X-chromosomal studies, the Ne for mtDNA and Y in particular, is below the expected median TMRCAs (See image Above and on the left). Y chromosome and mtDNA may be more representative of population structure immediately prior to expansion. However, meshing mtDNA TMRCA and Y TMRCA is problematic. If these two loci could be treated together, they would likely fall significantly below the X-linked and autosome-derived size estimates for any given TCHLCA.

    Most probable number of effective females based on TMRCA, showing the best estimate, and how Takahata's and Shaffners estimates compare (after conversion of Ne to Ne females

    Atkinson, Gray & Drummond (2009) show that prior to 150,000 years ago the population could have been as low as 1000 effective females (~1500 total, 4500 census) with a lower population size between 150,000 to 200,000 years ago. Whereas X-chromosome and autosomes warrant larger population size minima, 1000s of females, these loci of larger ploidy are capable of sensing population structure of much longer periods. Such periods may include recent and ancient population structures and size oscillations. Most population structure models for Africa have assumed much of the growth occurred very recently, however Atkinson et al. (2009) shows that by 100,000 years ago the minimum female population size exceed the estimated population size for females. The flat population/recent growth model is troubled in considering an ancient population core ine Tanzania (Gonder. et al. (2007) early East African/Khoisan split (Behar et al. 2008), and spread of L2 in parts of Africa where L0 and L1 are found in low abundance. Simply, the evidence of lineage growth appears to correlate with growth in geographic regions in which humans live. Retrospectively, this suggests that population size was growing as new lineages appears to expand territory. Comparing these observations with populations sizes suggested by X-chromosome (~7000 females) one might expect a low stand of the human population size of 1/3 to 1/2 this size between 150,000 to 250,000 years ago. This indicates that earlier periods had a reciprocal, or larger size (>7000 females) between 200,000 and 500,000 years ago.

    Other authors such as Endicott et al. (2009) think that bottlenecks in the human prehistory were such a common feature that they intefere with TMRCA determinations, and implies the possible effect of the OIS-6 on population size reduction with a TMRCA around the time of late pliestocene climate optimum, approximately 120,000 years ago.

    Geographic constraints of ancient humans

    The principal philosophical battle between strict Out of Africa and Multiregional Evolution hypotheses revolves around the placement of humans at times during human evolution. The singly interpretable result of mtDNA coalescence clearly favored a more recent African origins.

    The strict Out of Africa model places humans in sub-Saharan African or even more strictly, 1,000 to 20,000 interbreeding individuals. Consistent with the geographic distribution of phylogenetic reconstructions these individuals lived in a defined domain in sub-Saharan Africa for 1000s of generations between 100,000 and 250,000 years ago. Because all human females are considered to be within this time-space domain since other hominids (Neanderthals, Flores hobbit, Java man, Peking man, a set that also might include Jebel Irhoud) continue to evolve elsewhere. Which therefore indicates some fertility barrier existed between humans and these other types of humans, warranting the delineation of multiple human species. As part of this model specific events happened, population remains in a contained region, and at some point expands, expands out of Africa, expands to most parts of Africa, and since other hominids are no longer apparent, probably took part in a global-'competitive' displacement.

    In contrast, the strict multiregional hypothesis argues that humans were spread broadly across Africa, Eurasia, parts of Oceania. Humans interbreed overtime across long ranges, but modern humans primarily represent evolution in-situ. As part of this model the ice age ends allowing people to travel, agriculture increase population size, but people have largely evolved in place. Massive migrations and displacement would not explain genetic makeup.

    If we assume that there were humans in NE China, central China, southern China, Sumatra, Flores Island, Europe, the Levant, North Africa and Subsaharan Africa, and assuming there were no other humans other (e.g. Narmada India) then effective sizes per known regions was about 103 effective females (The more recent studies would suggest 100s of individuals per region between 150,000 and 200,000 years ago). In an Out of Tanzania model, 3000 individuals would be spread at densities of one per 300 square kilometers, at the size of sub-Saharan Africa under the OoA model this would mean that the density falls to one per 1000s of square kilometers and under the MREH model it would mean one per 10000s square kilometers. Based on relic stone age populations from around the world the recent African origin hypotheses better fit the estimated population sizes. As a consequence of increase information in support of OoA and the near impossibility of a strict MREH model many have repositioned their stance favoring a mostly Out of Africa hypothesis, in which modern humans recently migrated from Africa, but on rare occasion intermixed with regional humans (humans paraphyletic to Homo sapiens sapiens).

    Mitochondrial MRCA and the MRCA of all humans

    Mitochondrial Eve is the most recent common matrilineal ancestor, not the MRCA. Since the mtDNA are inherited maternally and recombination is either rare or absent, it is relatively easy to track the ancestry of the lineages back to a MRCA, however this MRCA is only valid when discussing mitochondrial DNA. Ironically mtDNA are not human, they are organelles that live within our cells, so it is better to say these are human-mitochondrial Most Recent Common Ancestor. Despite the recent fixation of the mtDNA genome in humans, other genes have evolved that were broadly selective in the human population, these genes have swept through the human population, two such genes have been identified on the X-chromosome. Other studies have indicated the overwhelming majority of humans have a recent common ancestor within the last 5000 years (albeit between any two individuals it may not be the same ancestor)[44], however the genetic relationship between well diverged individuals may not reflect the theoretical relationship, as geographic and cultural barriers may slow gene migration. Gene migration is not fluid in humans, as genes are passed in units called chromosomes, which undergo limited number of recombination on each unit per generation, therefore a common ancestor genealogically may not indicate the passage of DNA from that ancestor to the two divergent individuals. Whereas since mtDNA does not undergo this dilution via recombination, we can argue that the majority of mtDNA sequence (that which has not undergone mutation) from mtDNA ~16000 nts came from a single individual >150,000 years ago. A more recent common ancestor for all Males is the much larger Y chromosome (however it codes for very few genes).

    In popular science

    Cover of the January 11, 1988 edition of Newsweek

    Newsweek Magazine reported on Mitochondrial Eve based on the Cann et al. study in January 1988, under a heading of "Scientists Explore a Controversial Theory About Man's Origins". The edition sold a record number of copies.[45]

    Bryan Sykes has written a popular science book entitled The Seven Daughters of Eve (2001, ISBN 0-393-02018-5) that presents the theory of human mitochondrial genetics to a general audience.

    In River Out of Eden, Richard Dawkins discusses human ancestry in the context of a river of genes and shows that Mitochondrial Eve is one of the many common ancestors we can trace back to via different gene pathways.

    The Discovery Channel produced a documentary entitled The Real Eve (or Where We Came From in the United Kingdom), based on the book Out of Eden by Stephen Oppenheimer.

    In popular culture

    See also

    Notes

    1. ^ There are sites in mtDNA that evolve more rapidly such as the poly C region around CRS 16184 these regions have been noted to change within the individual, there are other 'hypervariable sites' like 16129, 16223, 16311, 16362 that flip flop frequently in human evolution- Excoffier and Yang. Mol. Biol. Evol. 16:1357-1368
    2. ^ This is described by Kimura and Wright as a Markov chain process, this process begins with 100% of an allele at absolute frequency of 1 (relative frequency = 1/2N), if the gene is excluded or fixes the Markov chain ends, but for all frequencies between 0 and 2N. For example, if the parent generation has relative frequencies of .1, .2, and .1 at absolute frequencies of 9,10, and 11, the probability of 12 individuals in the F1 generation would be 0.1*p(9->12) + 0.2*p(10->12) + 0.1*p(11->12) the calculation is performed for all possible absolute frequencies for the new generation based on frequecnies of the old generation and the new generation is replaced by to old and the process repeats
    3. ^ There are some fossil teeth at 9.8 Ma that might be proto-gorilla, there is one recent fossil for chimpanzee. Ardipithecus kadabba is credited by some as a CHLCA, however White et al. 2009 discounts this hypothesis claiming that the time of the CHLCA (TCHLCA is likely between 7 and 10 Ma, a period in which we have no potentially proto-hominid or proto-chimp fossils
    4. ^ "If man and old world monkeys last shared a common ancestor 30 million years ago, then man and African apes shared a common ancestor 5 million years ago..." Sarich & Wilson (1971)
    5. ^ Soares et al excluded 16182 and 16183 from their analysis
    6. ^ (CRS sites 16519, 152, 16311, 145, 195, 16189, 16129, 16083, 16362, 160, 709, 16129, 16083, 16362, 150, and 709)
    7. ^ It is also important to note, Eve as a female was not alone in the human population, while the modern population did not inherit their mitochondria from those other females, many other genes were passed from other loci, including X-linked and autosomal loci. A good example of a loci which maintained diversity are the HLA Loci. For HLA-B and HLA-DR there are hundreds of variants (alleles) mostly created through recombination. If one deconstructs these loci backwards to fundamental sets that are shared between multiple populations within and outside of Africa (with SNPs required to generate other alleles by recombination) one arrives at a dozen or more that must have been present during any population bottleneck. Since any individual can carry only 2, this implies many mating couples must have coexisted.

    Footnotes

    1. ^ Gonder et al. (2007), Ingman et al. (2000), Soares et al. (2009), Atkinson, Gray & Drummond (2009)
    2. ^ a b c d Gonder et al. (2007)
    3. ^ a b c Soares et al. (2009)
    4. ^ Dennett (1995). Darwin's Dangerous Idea. New York: Simon & Schuster. ISBN 0684802902. http://books.google.com/books?id=FvRqtnpVotwC&printsec=frontcover#PPA98,M1. 
    5. ^ see: Soares et al. (2009)
    6. ^ Kimura, M. (1962) On the Probability of Fixation of Mutant Genes in a Population. Genetics 47: 713–719.
    7. ^ Background for man: readings in physical anthropology, 1971
    8. ^ a b White TD, Asfaw B, Beyene Y, et al. (October 2009). "Ardipithecus ramidus and the paleobiology of early hominids". Science 326 (5949): 75–86. PMID 19810190. 
    9. ^ Arnason U, Gullberg A, Janke A (December 1998). "Molecular timing of primate divergences as estimated by two nonprimate calibration points". J. Mol. Evol. 47 (6): 718–27. doi:10.1007/PL00006431. PMID 9847414. 
    10. ^ a b see: Endicott et al. (2009)
    11. ^ a b Ingman et al. (2000)
    12. ^ See: Gonder et al. (2007),Soares et al. (2009)
    13. ^ Vigilant L, Pennington R, Harpending H, Kocher TD, Wilson AC (December 1989). "Mitochondrial DNA sequences in single hairs from a southern African population". Proc. Natl. Acad. Sci. U.S.A. 86 (23): 9350–4. doi:10.1073/pnas.86.23.9350. PMID 2594772. 
    14. ^ Vigilant et al. (1991)
    15. ^ Krings et al. (1997)
    16. ^ Suissa S, Wang Z, Poole J, Wittkopp S, Feder J, Shutt TE, Wallace DC, Shadel GS, Mishmar D. (2009). "Ancient mtDNA genetic variants modulate mtDNA transcription and replication.". PLoS Genet. 5 (5): e1000474. doi:10.1371/journal.pgen.1000474. PMID 19424428. PMC 2673036. http://www.plosgenetics.org/article/info%3Adoi%2F10.1371%2Fjournal.pgen.1000474. 
    17. ^ Balloux F, Handley LJ, Jombart T, Liu H, Manica A. (2009). "Climate shaped the worldwide distribution of human mitochondrial DNA sequence variation.". Proc Biol Sci. 276 (1672): 3447–55. doi:10.1098/rspb.2009.0752. PMID 19586946. 
    18. ^ a b Behar et al. (2008). "the dawn of human matrilineal diversity". The American journal of Human genetics 82 (5): 1130–40. doi:10.1016/j.ajhg.2008.04.002url=http://www.pubmedcentral.nih.gov/articlerender.fcgi?artid=2427203#app2 (inactive 2009-11-09). PMID 18439549. 
    19. ^ Ho SY, Larson G (February 2006). "Molecular clocks: when times are a-changin'". Trends Genet. 22 (2): 79–83. doi:10.1016/j.tig.2005.11.006. PMID 16356585. http://linkinghub.elsevier.com/retrieve/pii/S0168-9525(05)00335-5. 
    20. ^ Gibbons A (January 1998). "Calibrating the mitochondrial clock". Science 279 (5347): 28–9. doi:10.1126/science.279.5347.28. PMID 9441404. http://www.sciencemag.org/cgi/pmidlookup?view=long&pmid=9441404. 
    21. ^ Santos C, Sierra B, Alvarez L, Ramos A, Fernández E, Nogués R, Aluja MP. (2008). "Frequency and pattern of heteroplasmy in the control region of human mitochondrial DNA.". J Mol Evol. 67 (2): 191–200. doi:10.1007/s00239-008-9138-9. PMID 18618067. 
    22. ^ Excoffier L, Yang Z. (October 1999). "Substitution rate variation among sites in mitochondrial hypervariable region I of humans and chimpanzees.". Mol. Biol. Evol 16 (10): 1357–68. PMID 10563016. 
    23. ^ Wilson AC, Cann RL, Carr SM, et al (1985). "Mitochondrial DNA and two perspectives on evolutionary genetics". Biol J Linn Soc Lond. 26 (4): 375–400. doi:10.1111/j.1095-8312.1985.tb02048.x. http://www3.interscience.wiley.com/journal/119851665/abstract. 
    24. ^ Sykes, Bryan (2001). The Seven Daughters of Eve. New York: Norton. ISBN 0-393-02018-5. 
    25. ^ Brown WM (June 1980). "Polymorphism in mitochondrial DNA of humans as revealed by restriction endonuclease analysis". Proc. Natl. Acad. Sci. U.S.A. 77 (6): 3605–9. doi:10.1073/pnas.77.6.3605. PMID 6251473. 
    26. ^ Ferris SD, Brown WM, Davidson WS, Wilson AC (October 1981). "Extensive polymorphism in the mitochondrial DNA of apes". Proc. Natl. Acad. Sci. U.S.A. 78 (10): 6319–23. doi:10.1073/pnas.78.10.6319. PMID 6273863. 
    27. ^ See:Vigilant et al. (1989)
    28. ^ Reed FA, Tishkoff SA (2006). "Africa human diversity, origins and migrations". Current Opinions in Genetics & Development 16: 598. 
    29. ^ Tattersall I, Schwartz JH (2008). "The morphological distinctiveness of Homo sapiens and its recognition in the fossil record: Clarifying the problem.". Evol Anthropol 17: 49–54. doi:10.1002/evan.20153. 
    30. ^ Rightmire GP. (2009). "Out of Africa: Modern Human Origins Special Feature: Middle and later Pleistocene hominins in Africa and Southwest Asia.". Proc Natl Acad Sci U S A. 106 (38): 16046–50. doi:10.1073/pnas.0903930106. PMID 19581595. PMC 2752549. http://www.pnas.org/content/early/2009/07/02/0903930106.full.pdf. 
    31. ^ Takahata N (1993). "Allelic genealogy and Human Evolution". Mol. Biol. Evol. 10 (2): 2–22. PMID 8450756. 
    32. ^ See Reed & Tishkoff (2006),Zhou et al. (2006)Liu et al. (2006)
    33. ^ Takahate N (1993). "Allelic genealogy and human evolution". Mol Biol Evol 10 (1): 2–22. PMID 8450756. http://mbe.oxfordjournals.org/cgi/reprint/10/1/2. 
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    References

    External links

    Human mitochondrial DNA (mtDNA) haplogroups (by ethnic groups · famous haplotypes)

      most recent common mt-ancestor    
    L0 L1 L2 L3   L4 L5 L6
      M N  
    CZ D E G Q   A S   R   I W X Y
    C Z B F R0   pre-JT P  U
    HV JT K
    H V J T Former Clusters IWX

     
     
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