Star Cavalier
type of aircraft
The Star Cavalier was an American two-seat high-wing light aircraft first introduced in the late 1920s.
Development
The Star Aircraft division of Phillips Petroleum was formed at Bartlesville, Oklahoma in 1928. Designers E.A.Riggs and W.Parker prepared plans for a two-passenger high-wing light private owner aircraft intended for the lower cost end of the market. The advertised cost was $3,450. Three Cavalier A planes were delivered in 1928.
The Cavalier B followed in 1929 fitted with a lower powered 55 hp Velie M-5 engine and 15 examples were sold at $2,895 to owners of more modest means. Single examples of the Cavalier C and D followed. The next to secure modest success was the Cavalier E of 1930 which had a 90 h.p. Lambert and was fitted with a taller, more angular, tail fin. 13 were sold.
The public source identifies “Star Cavalier” as type of aircraft. This brief keeps that definition visible, then builds a research path around Star, Cavalier and type.
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Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Nov 8, 2025. The linked authority identifier is Q7600651. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1928, 1929 and 1930.
The absence of detail may reflect summary conventions rather than a lack of surviving documentation. The lead is largely declarative, so disagreement and counter-evidence require a deliberate search beyond the opening account. Authority statements aid reconciliation but still require their own references, qualifiers and ranks to be checked.
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This entry incorporates text from “Star Cavalier” on English Wikipedia. Contributors are listed in the page history. Text is available under the Creative Commons Attribution-ShareAlike 4.0 License. Selected authority identifiers and statements are retrieved from Wikidata under CC0; their references and qualifiers remain part of the verification path.