Ofatulena duodecemstriata
(Walsingham, 1884)
Twelve-lined Ofatulena
Ofatulena duodecemstriata is a tortricid in the tribe Grapholitini, first described by Walsingham in 1884 from the basionym Grapholitha duodecemstriata. The species is known by the "Twelve-lined Ofatulena" and has accumulated over 1,000 observations on iNaturalist, indicating it is a relatively well-documented member of its . It belongs to the Olethreutinae, a group of tortricid moths that includes many species associated with fruit and seed feeding. The specific epithet "duodecemstriata" refers to twelve stripes or lines, likely describing a diagnostic wing pattern feature.
Pronunciation
How to pronounce Ofatulena duodecemstriata: //oʊˌfætjuˈliːnə ˌduːoʊˌdɛkɛmˈstraɪətə//
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Identification
The name "duodecemstriata" (twelve-lined) suggests the presence of twelve longitudinal stripes or lines on the forewings, which may serve as a key diagnostic feature distinguishing this species from . As a member of the Ofatulena, it likely shares the general Grapholitini body plan with relatively narrow forewings and a characteristic resting posture with wings held in a tent-like or flattened position. Definitive identification requires examination of genitalia , as is standard for tortricid species discrimination.
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Similar Taxa
- Other Ofatulena species share similar body proportions and wing shapes, requiring careful examination of pattern elements (particularly the twelve-lined pattern implied by the specific epithet) and genitalia for reliable separation.
- Grapholita speciesFormerly classified in Grapholitha (now Grapholita), this may resemble other Grapholitini members in general appearance; the twelve-lined pattern and genitalic structure distinguish O. duodecemstriata.
More Details
Taxonomic history
Originally described as Grapholitha duodecemstriata by Walsingham in 1884, this was later transferred to the Ofatulena, reflecting refined understanding of relationships within the Grapholitini.
Observation frequency
With over 1,000 iNaturalist observations, this appears to be among the more frequently encountered members of its , though this may reflect observer effort and range rather than true abundance.