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Tāmaki River

Geography of AucklandHauraki Gulf catchmentRivers of New ZealandRivers of the Auckland Region
Rangitoto and Auckland 31 03 2012 14 03 10 cropped to Tamaki River
Rangitoto and Auckland 31 03 2012 14 03 10 cropped to Tamaki River

The Tāmaki River or Tāmaki Estuary is mostly an estuarial arm and harbour of the Hauraki Gulf, within the city of Auckland in New Zealand. It extends south for 15 kilometres (9 mi) from its mouth between the suburb of Saint Heliers and the long thin peninsula of Bucklands Beach, which reaches its end at Musick Point. The inlet extends past the suburbs of Glendowie, Wai o Taiki Bay, Point England, Glen Innes, Tāmaki, Panmure, and Ōtāhuhu to the west, and Bucklands Beach, Half Moon Bay, Farm Cove, Sunnyhills and Pakuranga to the east. It has several smaller "tributary arms" which extend from it: the Pakuranga Creek and Ōtara Creek in the east, and the Ōtāhuhu Creek and Panmure Basin in the west. The Ōtāhuhu Creek forms the eastern shore of the narrowest point on the Auckland isthmus: here it is about 1.25 kilometres (0.75 mi) to the waters of the Manukau Harbour, an arm of the Tasman Sea. It was originally called Te Wai o Taiki, meaning "The Waters of Taiki". The name Taiki is a shortened form of Taikehu, the name of an ancestor of Ngāi Tai.

Excerpt from the Wikipedia article Tāmaki River (License: CC BY-SA 3.0, Authors, Images).

Tāmaki River
Pakuranga Rotary Path, Howick Farm Cove

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Wikipedia: Tāmaki RiverContinue reading on Wikipedia

Geographical coordinates (GPS)

Latitude Longitude
N -36.8886826342 ° E 174.878482819 °
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Address

Pakuranga Rotary Path
2012 Howick, Farm Cove
Auckland, New Zealand
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Rangitoto and Auckland 31 03 2012 14 03 10 cropped to Tamaki River
Rangitoto and Auckland 31 03 2012 14 03 10 cropped to Tamaki River
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Farm Cove Observatory
Farm Cove Observatory

Farm Cove Observatory (FCO) is an amateur astronomical observatory in Pakuranga, Auckland, New Zealand, where Jennie McCormick discovered the main-belt asteroid 386622 New Zealand in September 2009.Built in 2000, the observatory has a Meade LX200R 14" Schmidt-Cassegrain F/10 telescope, purchased and on loan from Ohio State University Astronomy Dept. The observatory uses an SBIG ST8XME CCD camera with clear filter for data acquisition, this camera was supplied recently by the Centre for Backyard Astrophysics. FCO is only used for astronomical research. Farm Cove Observatory takes part in cataclysmic variable star (CV) research for the Center for Backyard Astrophysics and is also known as CBA Pakuranga. Up to January 2006, FCO has contributed over 1400 hours of data to the CBA, and the data from this observatory has been used in a number of scientific papers[1]. In April 2004 Farm Cove Observatory joined the MicroFUN collaboration [2] headed by Professor Andrew Gould at Ohio State University. The mission of MicroFUN is to obtain intense photometric monitoring of high magnification gravitational microlensing events in the hope of detecting planets orbiting the lensing star. Most of these events are found in the dense star fields of the bulge of the Milky Way galaxy. The first success came in April 2005 when an exoplanet was detected in the event OGLE-2005-BLG-071[3] [4]. The discovery was attributed to 31 professional astronomers and two amateurs. FCO contributed 12 hours of observations to this event. This new planet is about three times the mass of Jupiter and lies some 15,000 light-years toward the Galactic Bulge. This was only the second exoplanet detected by this technique and the first exoplanet discovery involving amateur observations. Recently, FCO has been contributing unfiltered magnitude measures to the British Astronomical Association campaign on Blazar OJ+287.