While visible as nebulous patch to the naked eye even under moderate conditions,
the Orion Nebula seems to have escaped pre-telescopic detection; only the bright
star Theta1 Orionis, which is situated within the nebula, was wellknown to
ancient and medevial astronomers. Even Galilei didn't mention it, although he
detected a number of stars in and around it during his first telescopic
observations in 1610, and in 1617, found the three brightest stars of the
Trapezium cluster.
A considerable number of consequent independent discoveries of this nebula
followed the invention of telescope:
Jesuit astronomer Johann Baptist
Cysatus of Lucerne (1588-1657) independently discovered it in 1611,
published in 1619 in his Mathemata astronomica de cometa anni 1618
(Cysatus 1619).
It was not before 1854 that Rudolf Wolf found and published Cysatus' discovery
(Wolf 1854).
Guillaume Bigourdan recovered
Peiresc's original discovery in 1916
(Bigourdan 1916), also referring to Cysatus'
finding, while Hodierna's work was rediscovered only in the 1980s
(Serio et.al. 1985).
References:
Guillaume Bigourdan, 1916.
La découverte de la nébuleuse d'Orion (N.G.C. 1976) par Peiresc.
Comptes Rendus, Vol. 162, pp. 489-490.
Giovanni Battista Hodierna, 1654.
De systemate orbis cometici, deque admirandis coeli characteribus
[About the systematics of the cometary orbit, and about the admirable
objects of the sky].
Palermo.
G.F. Serio, L. Indorato and P. Nastasi, 1985.
G.B. Hodierna's Observations of Nebulae and his Cosmology.
Journal of the History of Astronomy, Vol. XVI, No. 45, p. 1-36
(February 1985).
Rudolf Wolf, 1854.
Ueber den Nebelfleck im Orion.
Astronomische Nachrichten, Vol. 38, No. 859, col. 109/110.