Saturnia pyri

Superregnum: Eukaryota
Cladus: Unikonta
Cladus: Opisthokonta
Cladus: Holozoa
Regnum: Animalia
Subregnum: Eumetazoa
Cladus: Bilateria
Cladus: Nephrozoa
Cladus: Protostomia
Cladus: Ecdysozoa
Cladus: Panarthropoda
Phylum: Arthropoda
Subphylum: Hexapoda
Classis: Insecta
Cladus: Dicondylia
Subclassis: Pterygota
Cladus: Metapterygota
Infraclassis: Neoptera
Cladus: Eumetabola
Cladus: Endopterygota
Superordo: Panorpida
Cladus: Amphiesmenoptera
Ordo: Lepidoptera
Subordo: Glossata
Cladus: Coelolepida
Cladus: Myoglossata
Cladus: Neolepidoptera
Infraordo: Heteroneura
Cladus: Eulepidoptera
Cladus: Ditrysia
Cladus: Apoditrysia
Cladus: Obtectomera
Cladus: Macroheterocera
Superfamilia: Bombycoidea

Familia: Saturniidae
Subfamilia: Saturniinae
Tribus: Saturniini
Genus: Saturnia
Species: Saturnia pyri
Subspecies: S. p. pyri – S. p. thaumastos
Name

Saturnia pyri (Denis & Schiffermüller, 1775)
Synonyms

Bombyx pyri Denis & Schiffermüller, 1775 (original combination)

Vernacular names
Deutsch: Wiener Nachtpfauenauge
English: Great Peacock Moth, Large Emperor Moth, Giant Emperor Moth, Viennese emperor
español: Gran Pavón
suomi: Isoriikinkukkokehrääjä
français: Grand paon de nuit
magyar: Nagy pávaszem, nagy éjjeli pávaszem
svenska: Stor påfågelspinnare

Saturnia pyri, the giant peacock moth, great peacock moth, giant emperor moth or Viennese emperor, is a Saturniid moth which is native to Europe. The species was first described by Michael Denis and Ignaz Schiffermüller in 1775. It is the largest European moth, with a wingspan reaching 15–20 cm (6–8 in).

The giant peacock moth has a range that includes the Iberian Peninsula, southern France, northern Hungary, central and southern Serbia, Croatia, Montenegro, southern and eastern Bulgaria, southern Greece southern Turkey, south Kyrgyzstan, western Syria, Lebanon, north Israel, southern Romania, Russia, Ukraine, Czech Republic, Slovak Republic, Slovenia, North Macedonia and Italy and extends into Siberia and north Africa. It is absent from the UK, though a small handful of individuals have been recorded, likely of captive origin.[1]