Stardome Observatory (IAU observatory code 467, previously known as Auckland Observatory) is a public astronomical observatory situated in Cornwall Park in New Zealand's largest city, Auckland.
Founded in 1967, the observatory is administered by the Auckland Observatory and Planetarium Trust Board. The Trust Board was created by the Auckland Astronomical Society (AAS) in 1956. The Stardome Observatory is also home to the AAS.
In 1969, the observatory (then called Auckland Observatory) constructed a UBV photoelectric photometer with assistance from the University of Auckland. This photometer on the Zeiss telescope became a very successful instrument and produced a significant number of published research papers. Probably the most important discovery was the phenomenon of "super-humps" in the SU Ursae Majoris class of cataclysmic binary stars in 1974.
In 1988, the observatory participated in the discovery of the atmosphere of Pluto by measuring the brightness change as the planet passed in front of a star.
During the 1980s the Zeiss telescope was used to support several doctoral students from the University of Auckland (most notably Roger Freeth), including the development of a new computer-controlled photon counting photometer. Regular UBV photometry of variable stars continued until 1998 when a CCD camera was first used.
In 1999, a Celestron C-14 Schmidt-Cassegrain telescope was provided by the Nustrini family for installation in the newly built second dome at Stardome Observatory. A grant from the ASB Trust was used to buy a Paramount GT1100s mounting (manufactured by Software Bisque) and an Apogee AP8p CCD camera. The Apogee camera has a back-illuminated SITe003 CCD (1024×1024 24-micrometre pixels). The field of view is 22 arc-minutes. The 0.35 m (f/11) Nustrini telescope is used only for research. In 2006 the Celestron C-14 telescope was replaced by a 40 cm Meade ACF (F/10) and in 2008 CCD camera was replaced by a SBIG ST-6303. The Meade ACF telescope uses an OG530 Orange Schott Optical Glass Filter.