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Haplogroup E1b1b (Y-DNA)

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Author: Maciamo Hay.
Last update January 2017 (phylogenetic tree and history of M81)

Geographic distribution

Outside Europe, E1b1b is found at high frequencies in Morocco (over 80%), Somalia (80%), Ethiopia (40% to 80%), Tunisia (70%), Algeria (60%), Egypt (40%), Jordan (25%), Palestine (20%), and Lebanon (17.5%). On the European continent it has the highest concentration in Kosovo (over 45%), Albania and Montenegro (both 27%), Bulgaria (23%), Macedonia and Greece (both 21%), Cyprus (20%), Sicily (20%), South Italy (18.5%), Serbia (18%) and Romania (15%).

Distribution of haplogroup E1b1b in Europe, the Near East and North Africa

Distribution map of haplogroup E1b1b in Europe, the Near East and North Africa

Origins & History

East African origins

Haplogroup E1b1b (formerly known as E3b) represents the last major direct migration from Africa into Europe. It is believed to have first appeared in the Horn of Africa approximately 26,000 years ago and dispersed to North Africa and the Near East during the late Paleolithic and Mesolithic periods. E1b1b lineages are closely linked to the diffusion of Afroasiatic languages.

Lazaridis et al. (2016) tested the first ancient DNA samples from the Mesolithic Natufian culture in Israel, possibly the world's oldest sedentary community, and found that the male individuals belonged either to haplogroups CT or E1b1 (including two E1b1b1b2 samples). These are to date the oldest known E1b1b individuals. The same haplogroups show up in Pre-Pottery Neolithic Jordan, accompanied by new haplogroups (H2 and T). Besides, E1b1b was not found in Neolithic Iran or Anatolia, and only showed up twice among the hundreds of Neolithic European samples that have been tested. This suggests that agriculture did not originated with E1b1b tribes, but rather was brought by these H2 and T newcomers to the Levant. They would have blended with E1b1b people and together spread agriculture to the Arabian peninsula and North Africa.

The highest genetic diversity of haplogroup E1b1b is observed in Northeast Africa, especially in Ethiopia and Somalia, which also have the monopoly of older and rarer branches like M281, V6 or V92. Ethiopians and Somalians belong mostly to the V22 and V32 (downstream of V12) subclades, but possess also a minority of M81, M123 and V42 subclades. Among the main subclades of E1b1b only V13 and V65 are absent from the Horn of Africa, and probably originated in northern Africa (V65) or the southern Levant (V13).

Late glacial migration of E-M78 to Mediterranean Europe

It is still unclear when haplogroup E first entered Europe. The earliest known prehistoric sample to date is an E-V13 from Catalonia dating from 5000 BCE. So we know for sure that E1b1b was present in southern Europe at least since the Early Neolithic. Nonetheless, the possibility of other migrations of E1b1b to southern Europe during the Mesolithic or Late Palaeolithic cannot be ruled out. It is highly probable that the E-M78 subclade, found at relatively high frequencies in Mediterranean Africa, especially in Egypt (45% of the population) migrated to southern Europe before Neolithic herders from the Cardium Pottery culture arrived.

One might wonder why E1b1b is more common in the southern Balkans (Greece included) and southern Italy than anywhere in the Middle East, except in Egypt. What's more, the dominant form of E1b1b in Southeast Europe is E-V13, a subclade absent from the Horn of Africa and only present at low frequencies in North Africa (peaking in Lybia), the Levant and western Anatolia.

It has usually been assumed among academics that E-V13 and other E1b1b lineages came to the Balkans from the southern Levant via Anatolia during the Neolithic, and that the high frequency of E-V13 was caused by a founder effect among the colonisers. This theory has it that E1b1b people were associated with the development of Neolithic lifestyle and the advent of agriculture in the Fertile Crescent and its earliest diffusion to Southeast Europe (Thessalian Neolithic) and Mediterranean Europe (Cardium Pottery culture). The only concrete evidence for this at the moment is the presence of the E-V13 subclade, commonest in the southern Balkans today, at a 7000-year old Neolithic site in north-east Spain, which was tested by Lacan et al (2011). However, since E1b1b has not been found in any of the various Neolithic sites from the Balkans and Central Europe, it is more likely that the Catalan E-V13 individual was descended from Mediterranean Mesolithic hunter-gatherers.

This alternate hypothesis is that E-V13 migrated directly from North Africa to southern Europe, crossing the Mediterranean from Tunisia to Sicily, then to Italy and to the southern Balkans. This scenario would explain why E-V13 reaches its peak frequency just on the opposite side of the Strait of Otranto from Italy, i.e. in Albania (+ Kosovo) and Thessaly.

During the Ice Age, Malta, Sicily and mainland Italy formed a single land mass and the coast of North Africa was approximately half the distance it was today, making Sicily visible from Tunisia. Considering that Homo sapiens managed to get all the way to Australia by boat between 70,000 and 40,000 years ago, crossing the Strait of Sicily, perhaps via the small island of Pantelleria halfway, would have posed no major problem. In fact, it is almost certain that humans crossed that strait numerous times during the Stone Age.

Other subclades of E-M78 also present in North Africa and Europe today, like V12, V22 and V65, could also have crossed alongside V13. It is perhaps only due to a founder effect that V13 became considerably more common than other subclades in Europe, especially in the Balkans and eastern Europe. The greatest diversity of E-M78 subclades in Europe is actually found in Iberia, Italy and France, and not in the Balkans (where nearly all E1b1b are V13).

The Sahara changed many times from a lush green place to a hot and arid desert in the last 20,000 years. It was as arid as today at the end of the last Ice Age 13,000 years ago, then the warming climate brought tropical monsoons again from 10,000 to 7,000 years before present. The desertification taking place today started around 6,200 years ago. This series of severe transformations of their environment surely had a tremendous effect on the indigenous (E1b1b) people, causing populations booms during the green millennia following the Last Glacial Maximum, then again during the Neolithic period, and prompting migrations to milder climes once the rain had gone. The region most affected by the desertification would have been around modern Libya. The northern Maghreb enjoys the protection of the mountains that stopped the advance of the desert. Egypt had the Nile and its delta. As a result, if desertification did prompt North Africans to cross the Mediterranean at one time or another, they would most probably have crossed to Sicily first.

In such a scenario, North Africans would have belonged primarily to haplogroup E-M78. E-V13 is more common in Lybia today than anywhere in the Near East, which concords with central North Africa as being a potential source for the European E-V13 (and other subclades of M78). In fact, the small presence of E-V13 in the Near East could be better explained by the extremely long Greek presence in the eastern Mediterranean from the time of Alexander the Great until the end of the Byzantine domination over the region during the Middle Ages. It would be unthinkable that over 1,500 years of Hellenisation and Byzantine rule in Anatolia and the Levant didn't leave any genetic trace. In Anatolia, E-V13 is found mostly in the western third of the country, the region that used to belong to ancient Greece. The absence of E-V13 from Central Anatolia does not concord with a diffusion linked to Neolithic agriculture. There is clearly a radiation from the Greece (where E-V13 makes up approximately 30% of the paternal lineages) to the East Mediterranean (where the frequency drops to under 5%).

A strong argument in favour of E1b1b crossing directly from North Africa to southern Italy is that South Italians have more African admixture than people in the Balkans, Greece or Anatolia. This is true of the Northwest African admixture and the East African (Red sea) admixture. Another argument is that E1b1b has never been found among the dozens of Neolithic Y-DNA samples in the Balkans or Central Europe.

The Neoltihic farmers who migrated from the Levant to the Balkans would have brought mostly Southwest Asian admixture and apparently exclusively Y-haplogroup G2a. Many Neolithic sites yielded an occasional "outsider" to the G2a majority, but these were lineages (C1a2, F, I1, I2) that are thought to belong to assimilated (or enslaved) Mesolithic hunter-gatherers. That was very probably the case with E-V13 in Catalonia too.

The hypothesis of E1b1b settling in Mediterranean Europe since the Late Paleolithic or Mesolithic would also explain:

  • 1)...why South Italians and Iberians are more dolichocephalic (long-headed), like North Africans (although not as much), while North Italians (who are more of Italo-Celtic descent) are quite brachycephalic (broad-headed) like Central Europeans, Eastern Europeans and West Asians. A direct migration from North Africa to South Italy would have resulted not only in higher African admixture in South Italians, but also in a similar morphology. The Greeks are intermediary because they would have been blended with broad-headed West Asian Neolithic farmers (G2a) and later Bronze Age invaders (Indo-European R1a and R1b, but also Anatolian J2). Further north in the Balkans, the Mediterranean dolicocephalic type were supplanted by the Eastern European, Central Asian and West Asian brachycephalic type over time due to the numerous migrations to the region.

  • 2)...the almost complete absence of other Paleolithic lineage (notably I2) from southern and central Italy, except in Sardinia, which was presumably not settled by Paleolithic North Africans due to its distance from the nearest coast. It would rather have been settled through Corsica from North Italy by Central European hunter-gatherers (I2a1). The modern Sardinian population distinguishes itself by its higher frequency of non-Mediterranean Mesolithic ancestry (such as WHG) but the nearly complete absence of East African admixture. Sardinia is also the only region of Italy which almost doesn't have any E-V13.

    In the Balkans, I2a1b lineages only came between the Bronze Age (Thracians, Illyrians) and the Middle Ages (Slavs). If haplogroups C, F and I were the only Paleolithic European lineages, why would indigenous Paleolithic lineages be wiped out from the Balkans and most of Italy with the arrival of Near Eastern farmers, but survive and remain the dominant lineage in Sardinia, which was an important Neolithic centre belonging to the same Cardium Pottery culture as the rest of Italy ? The best explanation is that E1b1b was already the dominant Paleolithic lineage in the Balkans and Italy, apart from Sardinia, and therefore Paleolithic lineages weren't wiped out, but assimilated by Neolithic farmers, which assured their survival.

Assimilation of E-M78 by Neolithic farmers

Even if E1b1b was not one of the original lineage of Near Eastern Neolithic farmers, its presence in southern Europe during the Mesolithic would have brought it into contact very early on with agriculture. It has been confirmed that at least some E-V13 people were assimilated by G2a farmers of the Cardium Pottery culture, which started in Italy and spread to southern France and Iberia. However, out of 27 Neolithic Y-DNA samples derived from the Thessalian Neolithic (Starčevo culture and Linear Pottery culture), no a single one of them belonged to E1b1b. This could either mean that E-V13 was present in the Balkans, but lived as hunter-gatherers in other regions than farmers, or that E-V13 only entered the Balkans later in the Neolithic from Italy, after Italian E-V13 adopted agriculture during the Cardium Pottery period.

Nowadays E1b1b is the only Mediterranean haplogroup consistently found throughout Europe, even in Norway, Sweden, Finland and Baltic countries, which are conspicuous by the absence of other Neolithic haplogroups like G2a (bar the Indo-European G2a3b1), J1 and T (except in Estonia). However, since G2a is the only lineage that was consistently found in all Neolithic sites tested to date in Europe, the absence of Neolithic G2a lineages from Scandinavia and the Baltic implies that no Neolithic lineage survives there, and consequently E1b1b (mostly E-V13) does not date from the Neolithic in the region. It could easily have been brought by the Indo-European invasions during the Bronze Age, as a minority lineage picked up in Southeast Europe by the R1b tribes before they made their way to Central Europe and eventually Scandinavia. At present the most consistent explanation is that E-M78 was indigenous to southern Europe in the Mesolithic, and was assimilated by G2a farmers, then by R1b Indo-Europeans. There is in fact a very low diversity among E-V13 in central and north-east Europe, which is consistent with a relatively recent (Bronze to Iron Age) dispersal from a common source.

North African Neolithic cattle herder hypothesis

Decker et al (2013) reported that Iberian and Italian cattle possess introgression from African taurine, which could imply that cattle were not just domesticated in West Asia, but also independently in North Africa. If that is the case, E-M78, and notably E-V13, could have come to southern Europe through North African cattle herders during the Neolithic, although this hypothesis remains purely conjectural.

The origins of E-M81: Carthaginian, Roman or Moorish?

Nowadays E-M81 is the dominant paternal lineage among Maghrebans, and particularly Tunisians and Mountain Moroccans. Outside North Africa, M81 is far more frequent in parts of Iberia than anywhere else in Europe or the Near East. The M81 clade is defined by 150 other mutations beside M81 itself. This branch split from E1b1b during the late glacial period, approximately 14,000 years ago. It would be easy to assume that E-M81 colonised Northwest Africa during the Mesolithic or Neolithic period, then spread to southern and western Europe with the southern wave of Neolithic farmers that crossed over from Morocco to Iberia, then spread around western Europe with the Megalithic people. Yet, according to TMRCA (Time of Most Recent Common Ancestor) estimates, all carriers of this haplogroup descend from a common ancestor who lived only 2,100 years ago, about 5,000 years too late for the Neolithic hypothesis to hold ground.

The story of M81 is very unusual in that it is so young and diversified into a multitude of subclades within just a few centuries. M81 has two immediate subclades A5604 and M183 (aka PF2477 or PF2546). Under the latter no less than eight subclades have been identified at present: A930, A2227, CTS12227, FGC22844, PF2578, PF6794, MZ99 and Z5009. This indicates that a single man may have had nine sons who went on to have numerous children of their own. What is even more surprising is that these subclades do not show any consistent geographic pattern.

If the estimate of 2,100 years is correct, that would correspond approximately to the time when the Romans defeated the Carthaginians in what is now Tunisia. That would mean that the M81 lineage only started to expand in Roman times, and continued to diffuse within all the borders of the Roman Empire - not just North Africa, but also Iberia, France, Italy, Greece, Turkey and the Levant. This is a remarkably fast expansion that would have required a male line of considerable wealth and influence within the Roman Empire, and therefore probably a family of rich patricians or even a Roman emperor, not necessarily of Roman descent himself. The advantage of this hypothesis is that M81 is indeed found exclusively within the borders of the Roman Empire, and in a big part of the empire. Even within Britain it is found mainly in Wales, a region known to have served as a refuge for the Romano-British population during the Anglo-Saxon invasions.

Of course, the TMRCA is only an estimate and could vary by a few centuries. Therefore this lineage could actually have emerged a few centuries earlier, during the Phoenician/Carthaginian period. Indeed the distribution pattern and frequency of M81 matches much better the Phoenician maritime empire, with its origins in the Levant, and its dispersal along the cost of North Africa, but also Iberia, Sardinia and Sicily. In this scenario, M81 could have been the lineage of Carthaginian kings, or of a particularly prolific aristocratic familiy during the Carthagininan Republic. The merits of this hypothesis is that it would explain why M81 is so much more common in the Maghreb, and particularly in Tunisia, than in Italy today. The Carthaginians founded cities in Spain, including Carthago Nova (the New Carthage, now Cartagena in Murcia), but also in Sardinia and Sicily, where M81 is the most common today within Italy. The weak point of this hypothesis is that it doesn't explain how M81 reached places like France, Britain, Greece or Turkey, nor even northern Spain.

In whichever scenario, it is clear that M81 benefited from a potent founder effect in the Maghreb, a region that was first dominated by the Carthaginian elite, but quickly became one of the favourite regions of residence for the Roman elite within the empire (along with Spain, France and Greece). Therefore both hypotheses are plausible. A combination of the two scenarios could provide an even better explanation. M81 would first have spread with the Carthaginian elite, then once they were defeated by the Romans and annexed to the empire, their descendants would have been free to migrate to various parts of the empire from North Africa, Sicily, Sardinia and Iberia, some eventually reaching France and Britain. The original Phoenician M81 in the Levant could also have diffused across the Eastern Mediterranean over the centuries, during the Roman, Byzantine and Ottoman periods.

Whether origins of M81 lie in the Carthaginian or Roman elite, its parent clades M310.1 and Z827 would have originated in the Levant, and not in Northwest Africa. M310.1's sister clade, Z830 is almost exclusively Middle Eastern. M310.1 itself dates from the Late Paleolithic and could have come to Italy via Anatolia and Greece any time between the Late Glacial period and the Iron Age, including with Neolithic farmers, the Minoans, or the Etruscans.

In either case, it is likely that more M81 came into the Iberian peninsula during the Moorish period, when the Maghrebian Arabs conquered most of what is now Spain and Portugal, where they remained for over 700 years. The Moors also conquered Sicily.

Phoenician, Greek and Roman diffusions of E1b1b

The classical antiquity brought new waves of colonisation across the Mediterranean. The first colonists were Phoenicians, who came from present-day Lebanon and the Tartus province of Syria. The Phoenicians possessed a variety of paternal lineages reflecting the complex ancient history of the Middle East. One of them was E-M34, which makes up about 15% of modern Lebanese Y-DNA, but was probably a higher before the Greek, Roman, Arabic, Byzantine, medieval crusader and Ottoman occupations. E-M34 is the main Middle Eastern variety of E1b1b and is thought to have arrived with the Proto-Semitic people in the Late Copper to Early Bronze Age. The Phoenicians would have spread E-M34 to Cyprus, Malta, Sicily, Sardinia, Ibiza and southern Iberia.

The ancient Greeks contributed to the rediffusion of more E-V13 around places such as Cyprus, Sicily, southern Italy, Liguria, Provence, eastern Spain, and basically all part of the Classical ancient Greek world. Alexander's conquest of the Middle East would have taken E-V13 much further afield, perhaps as far as Afghanistan and Pakistan, although only at trace frequencies. The Greeks remained in control of the Middle East until the Roman conquest, then regained influence over the region during the Byzantine period. It is likely that most E-V13 in the Middle East is ultimately of Greek origin.

The Etruscans, who may have come from western Anatolia, could have brought E-M34 and more E-V13 to central Italy, which would then have been assimilated by the Romans. Migrations within the Roman Empire probably played a role, although a minor one, in the redistribution of E1b1b in Europe. The biggest genetic impact of the Romans/Italians outside of Italy appears to have been in Gaul (modern France, Belgium, southern Germany and Switzerland), probably because this was the closest region to Italy using the well-developed Roman road network (actually inherited from the Gauls themselves).


Phylogenetic tree of haplogroup E1b1b (Y-DNA) - Eupedia

Phylogenetic tree of haplogroup E-V13 (Y-DNA) - Eupedia

Five major subclades of E1b1b (V12, V13, V22, M81, M123) originated in Northeast Africa before the Neolithic. Consequently most of them are present virtually in all regions where E1b1b is found. One exception is Norway, Sweden and Finland, where only E-V13 seems to be present.

The frequency of E subclades has varied geographically over time due to founder effects in Neolithic populations, i.e. the migration of a small group of settlers carrying among whom one paternal lineage was much more common than any others. Examples of founder effects include E-V12 in southern Egypt, E-V13 in the Balkans, E-V32 in Somalia, E-V65 on the Mediterranean coast of Africa, and E-M81 in Northwest Africa.

E1b1b1a1 (M78)

E-M78 is the most common variety of haplogroup E among Europeans and Near Easterners. E-M78 is divided into 4 main branches : E1b1b1a1 (E-V12), E1b1b1a2 (E-V13), E1b1b1a3 (E-V22) and E1b1b1a4 (E-V65), each subdivided in further subclades.

  • E-V13
    • The E-L17 subclade has been found from Ukraine to Portugal and from Sardinia to England.
    • The E-L143 subclade has only been found in England.
    • The E-L241 subclade has been found in the Czech Republic and England.
    • The E-L540 subclade has been found in Germany, the Czech Republic, Poland, Belarus and Sweden.

Distribution of haplogroup E-V13 in Europe, the Middle East & North Africa

Distribution map of haplogroup E-V13

  • E-V22 is found primarily in western Ethiopia, northern Egypt and in the southern Levant. In Europe it is therefore associated with the Phoenicians and the Jews. The Phoenicians could have disseminated E-V22 to Sicily, Sardinia, southern Spain and the Maghreb, and the Jews to Greece and mainland Italy and Spain. However, V22 might have been found among Mesolithic South Europeans like V13.

  • E-V12 is the most common subclade of M78 in southern Egypt (over 40% of the population), while its V32 subclade is the dominant paternal lineage in Somalia, southern Ethiopia and northern Kenya. The moderate presence of V12* in the Near East and across Europe (except Nordic countries) indicates that it could have been a minor Mesolithic South European lineage accompanying E-V13. Its V32 subclade has not been found outside Northeast Africa.

  • E-V65 is found chiefly in North Africa, with a maximum frequency (20-30%) observed in Lybia, Tunisia and northern Morocco. The absence of V65 from the Horn of Africa means that it would have originated in North Africa. V65 has also been found at lower frequencies (0.5% to 5%) in Egypt, Greece, southern Italy, Sicily, and more interestingly among the Sardinians and the Basques, two population isolates with strong affinities with the Neolithic and Mesolithic populations of Europe, but both mostly lacking E-V13. However, V65 has not been found in the Levant, the Balkans or in non-Mediterranean Europe, which disproves a Neolithic dispersal. Its strongly North African distribution and very minor presence in parts of southern Europe with historical links to North Africa would rather suggest that this lineage was brought to southern Europe by immigrants from North Africa. In the case of Italy this could have taken place any time from the Phoenician/Carthaginian period (c. 1000-146 BCE) until the Vandal Kingdom. In Greece, V65 could have come from the ancient colonies of Cyrenaica. In Iberia, V65 could have crossed the Strait of Gibraltar any time since the late Paleolithic.

E1b1b1b1a (M81)

E-M81 probably originated in the Horn of Africa, although its presence is very limited there nowadays (1.5% in Somalia, 5% in Sudan). M81 spread throughout North Africa and the Levant, and became the dominant lineage of the Berbers of Northwest Africa, almost certainly due to a founder effect. M81 is found at an average frequency of 45% in the Maghreb and Lybia, with peaks at over 60% in Tunisia as well as central and southern Morocco. M81 is also found in Portugal (8%), Spain (4%), as well as in France (0-6%) and Italy (0-4%), where strong regional variations are observed. M81 is especially common in western Iberia, notably Extremadura (15.5%), Andalusia (13.5%), southern Portugal (11%), north-west Castille (10%) and Galicia (10%). The highest percentage of E-M81 in Europe is found among the Pasiegos (30%, n=101), an isolated community living in the mountains of Cantabria.

Note the resemblance between the distribution of E-M81 and the African admixture from the Dodecad project.

Distribution of haplogroup E-M81 in Europe, the Middle East & North Africa

Distribution map of haplogroup E-M81

E1b1b1b2a (M123)

E-M123 is most commonly found in Ethiopia (5-20%), where it appears to have originated. Its main subclade E-M34 probably emerged in the southern Levant, where it reaches its maximum frequency (10-12% among the Palestinians and the Jews, 8% among the Bedouins, 5% in Lebanon), then expanded in every direction across North Africa (3-5%), the Middle East and South Asia, Anatolia (3-6%) and southern Europe, particularly Italy (1 to 8%).

In Europe E-M123 is only observed at frequencies over 2.5% in southern Italy, in the Spanish region Extremadura (4%), and the Balearic islands of Ibiza and Minorca (average 10%). E-M123 could have been brought to the Mediterranean coasts of Europe by the Phoenicians, and to Italy by the Etruscans (from Anatolia). The Romans might have contributed to spreading it around their empire at low frequencies.

E-M34 is the most common form of E1b1b among Jewish people. Based on the few people who tested for tested for deeper subclades, Jewish people can either belong to the M84 or the L791 subclade of M34.

The M293 (aka CTS2297) subclade of M34 has been found among Arabic people from the Arabian peninsula (Kuwait).

Distribution of haplogroup E-M123 in Europe, the Middle East & North Africa

Distribution map of haplogroup E-M123

Famous individuals

E-V13 branch

The Wright Brothers, the inventors of the world's first successful airplane, belonged to haplogroup E-V13. They were supposedly descended from Robert Wright of Brook Hall, Essex, England, which allowed the Wright Surname DNA Project to isolate their paternal lineage.

Lyndon B. Johnson (1908-1973), the 36th President of the United States, was identified as a member of haplogroup E1b1b1 through the Johnson/Johnston/Johnstone DNA Surname Project. His haplotype, although not confirmed by SNP testing yet, is predicted as E-V13.

E-M34 branch

The Harvey Y-DNA Genetic Project managed to retrace the ancestry and identify the Y-chromosomal haplogroup of William Harvey (1578 -1657), the first person to describe completely and in detail the systemic circulation and properties of blood being pumped to the body by the heart. He belonged to the subclade E-M34.

Gérard Lucotte et al. (2012) recovered the DNA of Napoleon Bonaparte from beard hair follicules and compared his Y-DNA to that of one of his present-day descendants, Charles Napoléon. They established that both men belonged to haplogroup E-M34, a subclade which is thought to have reached Mediterranean Europe from the Levant during the Neolithic period. Napoleon I had previously been identified by Lucotte's team as a member of mtDNA haplogroup H.

The acclaimed theoretical physicist Albert Einstein is presumed to have belonged to Y-haplogroup E-Z830 based on the results from a patrilineal descendant of Naphtali Hirsch Einstein, Albert Einstein's great-grand-father. Approximately 20% of Ashkenazi Jews belong to haplogroup E1b1b.

Steven Pinker (Photo by Rebecca Goldstein - CC BY-SA 3.0)

Steven Pinker is a Canadian experimental psychologist, cognitive scientist, linguist, and popular science author. He is Johnstone Family Professor in the Department of Psychology at Harvard University, and is known for his advocacy of evolutionary psychology and the computational theory of mind.

Cage at the 2011 San Diego Comic-Con International (CC BY 2.0)

The American actor and producer Nicolas Cage (born 1964),has been found to belong to haplogroup E1b1b-M84. His real name is Nicolas Kim Coppola, and his paternal great-grand-father emigrated to the U.S. from the South Italian town of Bernalda in Basilicata. He is the nephew of screenwriter, film director and producer Francis Ford Coppola, who shares the same haplogroup.

E-M81 branch

Zinedine Zidane (CC BY 2.0)

The French footballer of Algerian origin Zinedine Zidane (born 1972), is a member of haplogroup E1b1b (M81) according to his brother's DNA test. Zidane was named the best European footballer of the past 50 years in the UEFA Golden Jubilee Poll.

Undetermined E1b1b branch

The great Italian Baroque painter Caravaggio (1571-1610) were excavated to confirm the circumstances of his mysterious death at the age of 38. His DNA was compared to modern carriers of the same surname. The study revealed that he belonged to haplogroup E1b1b1.

Ronny Decorte, a geneticist from the Catholic University of Leuven in Belgium, tested relatives of Adolf Hitler and determined that the Fürher belonged to haplogroup E1b1b. Ironically this haplogroup thought to be at the origin of Afro-Asiatic languages, which includes the Semitic languages and peoples that Hitler despised so much.

Richard Attenborough (Photo by gdcgraphics - Creative Commons Attribution 2.0 Generic license.)

Sir David Attenborough (b. 1926), an English broadcaster and naturalist at the BBC explained in the Tree of Life how the Attenboroughs belonged to haplogroup E1b1b1. In 2002 he was named among the 100 Greatest Britons following a UK-wide vote. His brother is the producer, director and actor Richard Attenborough (b. 1923 - pictured), who won two Academy Awards for Gandhi in 1983.

Other famous members of haplogroup E1b1b

  • Tom Conti (subclade E-M34) : is a Scottish actor, theatre director and novelist of Italian Scots descent. He has won a Tony Award for Best Actor in a Play in 1979 for his performance in Whose Life Is It Anyway? His haplogroup was revelaved to be E-M34 by BritainsDNA.
  • George Stroumboulopoulos : is a Canadian television and radio personality. He is best known as formerly being a VJ for the Canadian music television channel MuchMusic and being the host of the CBC Television talk show George Stroumboulopoulos Tonight (formerly The Hour) from 2005 to 2014.

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