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Carambola, also known as star fruit, is the fruit of Averrhoa carambola, a species of tree native to tropical Southeast Asia. [1] [2] [3] The edible fruit has distinctive ridges running down its sides (usually 5–6). [1] When cut in cross-section, it resembles a star, giving it the name of star fruit.
Averrhoa carambola is a species of tree in the family Oxalidaceae native to tropical Southeast Asia; [1] it has a number of common names, including carambola, star fruit and five-corner. [2] It is a small tree or shrub that grows 5 to 12 m (16 to 39 ft) tall, with rose to red-purple flowers.
The North Star cherry is a sour cherry tree. [1] A dwarf cultivar, it typically grows 8 to 10 feet tall. [2] Both the skin and flesh are a deep red. The North Star is excellent for baking, and makes superb wine. Developed by the University of Minnesota, (the "North Star State"), [3] [4] [5] it is self-pollinizing (meaning only one tree is ...
Star Distance ly Notes 1 Proxima Centauri: 4.2 ly (1.3 pc) Part of the α Cen trinary system, the closest neighbouring star system. It is also the nearest neighbouring star. [9] 2 Barnard's Star: 5.95 ly (1.82 pc) Second closest neighbouring star system [16] 3 Wolf 359: 7.86 ly (2.41 pc) Also called CN Leonis: 4 Lalande 21185: 8.3 ly (2.5 pc) 5
A K-type main-sequence star, also referred to as a K-type dwarf, or orange dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars ("red dwarfs") and yellow/white G-type main-sequence stars .
Amphipholis squamata, common names brooding snake star and dwarf brittle star, is a species complex [2] [3] of brittle stars in the family Amphiuridae. [ 4 ] [ 5 ] [ 6 ] Description
A. hispida's small size, especially when compared to its Angophora and Eucalyptus relatives, leads to it being known by the common name dwarf apple. [1] It is native to a relatively small patch of central New South Wales – from just south of Sydney up to the Gosford area.
White dwarfs are stellar remnants produced when a star with around 8 solar masses or less sheds its outer layers into a planetary nebula. The leftover core becomes the white dwarf. It is thought that white dwarfs cool down over quadrillions of years to produce a black dwarf. [14] Neutron star: RX J0720.4−3125: 0.0000064683 – 0.0000077332
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