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A pet blanket constructed from a single granny square with a shell stitch border, enhanced in a contrasting color with half double crochet. The basic method of producing shell stitches is to anchor several long stitches into the same base, anchoring both ends with short stitches in a manner that spreads out the cluster like a fan. Although many ...
Crochet hooks used for Tunisian crochet are elongated and have a stopper at the end of the handle, while double-ended crochet hooks have a hook on both ends of the handle. Tunisian crochet hooks are shaped without a fat thumb grip and thus can hold many loops on the hook at a time without stretching some to different heights than others (Solovan).
The Melotte catalogue is a catalogue of 245 star clusters compiled by British astronomer Philibert Jacques Melotte.It was published in 1915 as A Catalogue of Star Clusters shown on Franklin-Adams Chart Plates. [1]
See also: Open cluster, List of open clusters NGC 1662 (also known as Collinder 55 ) is a loosely bound open cluster located in the constellation Orion . It has an apparent magnitude of 7.6 [ 1 ] and an approximate size of 20 arc-minutes .
NGC 2244 (also known as Caldwell 50 or the Satellite Cluster) is an open cluster in the Rosette Nebula, which is located in the constellation Monoceros. This cluster has several O-type stars , super hot stars that generate large amounts of radiation and stellar wind .
Messier 71 (also known as M71, NGC 6838, or the Angelfish Cluster) is a globular cluster in the small northern constellation Sagitta. It was discovered by Philippe Loys de Chéseaux in 1745 and included by Charles Messier in his catalog of non- comet -like objects in 1780.
IC 4756 is a large bright open cluster in the constellation Serpens. Known as Graff's Cluster, it is bright enough to be seen with the naked eye and considered a fine cluster for binoculars or small telescopes. [2] IC 4756 is also known as the Tweedledee Cluster (paired with NGC 6633 as Tweedledum), also as the Secret Garden Cluster. [3]
The cluster lies between the constellation Crux and the larger but fainter "False Cross" asterism. The 4th-magnitude Cepheid variable star x Carinae appears near the southeast fringes, but it lies between the Sun and the cluster and is not a member of the cluster. The cluster was first catalogued by Nicolas Louis de Lacaille in 1752. [18]
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