Barbary falcon

Barbary falcon
Not recognized (IUCN 3.1)
Scientific classification
Kingdom: Animalia
Phylum: Chordata
Class: Aves
Order: Falconiformes
Family: Falconidae
Genus: Falco
Species: F. pelegrinoides
Binomial name
Falco pelegrinoides
Temminck, 1829

The Barbary falcon (Falco pelegrinoides) is a medium-sized falcon about the size of a crow. This bird of prey is mainly resident.

Description

The Barbary falcon is a bird of semi-desert and dry open hills. It typically lays its eggs in cliff-ledge nests.

It is similar to the peregrine falcon, but smaller at 33–39 cm length with a wingspan of 76–98 cm. The female is larger than the male. It resembles its relative in general structure.

Adults have paler grey-blue upperparts than the peregrine, and often have a buff wash to the barred underparts, whereas the larger species has a white background color. The nape is rufous, but this is difficult to see.

Sexes are similar, apart from size, but the young birds have brown upperparts and streaked underparts. The streaking is lighter than in the juvenile peregrine.

The call is a high-pitched "rek-rek-rek".

The Barbary falcon also bears some resemblance to the lanner falcon, but can be distinguished from that species at rest by the head-pattern, and in flight, by the proportions, flight action and underwing pattern.[1]

Barbary falcon

Distribution

The Barbary falcon is native to Northern and Eastern parts of Africa (Algeria, Canary Islands, Egypt, Eritrea, Morocco, Niger, Sudan, Somalia, Tunisia and Yemen). It is also common in Middle East, Central Asia and South Asia, particularly in Afghanistan, China, India, Iran, Iraq, Israel, Jordan, Kazakhstan, Kuwait, Kyrgyzstan, Libya, Oman, Saudi Arabia, Syria, Tajikistan, Turkmenistan, United Arab Emirates and Uzbekistan. It is vagrant in Burkina Faso, Cameroon, Djibouti, Greece, Italy, Kenya, Lebanon, Mali, Malta, Nepal, Portugal, Qatar, Senegal and Turkey.[2]

Taxonomy

The Barbary falcon differs in appearance from the peregrine falcon according to Gloger's rule. The genetic distance is slight and the species form a close-knit and somewhat paraphyletic group in DNA sequence analyses. In fact, some taxonomic authorities consider it conspecific. They differ more in behavior, ecology and anatomy[3] than usual for conspecifics. They are able to produce fertile hybrids,[4] but they are generally allopatric and only co-occur during breeding season in small areas such as the Maghreb,[5] the Punjab, Khorasan, and possibly the Mongolian Altai, and there is clear evidence of assortative mating with hybridization hardly ever occurring under natural conditions. In short, though they occupy adjacent territories, they breed at different times of year and Barbary falcons virtually never breed with peregrines in nature.[6][7][8][9][10][11][12]

Assuming a genetic distance of 2% in hierofalcons[12] corresponds to a divergence roughly 200,000–130,000 years ago,[13] the 0.6–0.7% genetic distance in the peregrine-Barbary falcon ("peregrinoid") complex [11] suggests its current taxa evolved in the Late Pleistocene some 100,000 years ago or less, but before the Upper Paleolithic. The presumed time of divergence between peregrine and Barbary falcons approximately coincides with the start of the last ice age, when desertification was prominent in North Africa and the Middle East, and the Persian Gulf became a landlocked inland sea that slowly dried up. Populations of ancestral "peregrinoid" falcons living in marginal habitat at the fringe of the African-Middle Eastern desert belt either adapted (and might have become isolated e.g. in the Persian Gulf region, which turned into semiarid habitat surrounded by vast deserts), or left for better habitat, or became extinct. During interstadials, deserts receded and the aridland and humidland populations could expand to contact again, causing some limited gene flow. This scenario by and large parallels the proposed evolutionary history of the saker falcon in relation to the other hierofalcons; indeed, that group shows similar patterns of molecular paraphyly though it is of somewhat earlier origin.[13]

The fossil record adds little to the issue. A humerus some 9,000 years old (i.e., after the last ice age) from the Aswan area in Sudan, where Falco peregrinus minor occurs today, was identified to belong to the peregrine.[14] The Barbary falcon is one of the rare cases that may arguably be considered a species under the biological species concept, but certainly not under the phylogenetic species concept rather than the other way around as usual. This case demonstrates that what makes a "species" is not only its descent, but also occurs to a population in the course of evolution, how it adapts, and how this affects its reproductive isolation (or lack thereof) from sister taxa.

Notes

  1. ↑ Clark & Shirihai (1995)
  2. ↑ BirdLife International (2012). "Falco pelegrinoides". IUCN Red List of Threatened Species. Version 2013.2. International Union for Conservation of Nature. Retrieved 26 November 2013.
  3. ↑ Notably, the Barbary falcon has a peculiar way of flying, beating only the outer part of its wings like fulmars sometimes do; this also occurs in the peregrine, but less often and far less pronounced (Snow et al. 1998). The Barbary falcon's shoulder and pelvis bones are unusually stout by comparison with the peregrine and its feet are smaller (Vaurie, 1961), suggesting that hybridization has not affected the evolution of these traits. It was proposed (Vaurie, 1961) that the Barbary falcon also has an elongated middle toe, but this seems to be in error (Snow et al. 1998).
  4. ↑ White (1994), though as seen above, fertile hybrids may occur between peregrine falcons and undoubtedly good and far more distant species. In general terms, the ability to produce fertile offspring is a plesiomorphy initially shared by close relatives; the loss of ability to hybridize successfully is an apomorphy. Hence, the inability rather than the ability to produce fertile hybrids is phylogenetically informative.
  5. ↑ Schollaert & Willem (2000)
  6. ↑ Vaurie (1961)
  7. ↑ Helbig et al. (1994)
  8. ↑ Snow et al. (1998)
  9. ↑ Wink et al. (1998)
  10. ↑ Wink & Sauer-Gürth (2000)
  11. 1 2 Wink et al. (2000)
  12. 1 2 Wink et al. (2004)
  13. 1 2 Nittinger et al. (2005)
  14. ↑ Tchernov (1968)

References

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