Vy Ursae Majoris

On the other hand it stays relatively bright throughout its irregular period ranging from magnitude 5 9 to 7 0 so it should be an easy target for binocular users. The bright star catalogue 5th revised ed.

Vy Canis Majoris Constellation Guide

Vy canis majoris is surrounded by a complex asymmetric circumstellar envelope caused by mass loss from the star itself.

Vy ursae majoris. Beljawsky during his investigation of simeiz observatory plates. Carbon star vy ursae majoris click the full screen zoom button click the image to. Lalande 21185 is a red dwarf star type m2 positioned in southern ursa major close to the leo minor constellation boundary.

Vy canis majoris is a pulsating variable star situated at around 3 900 light years 1 2 kiloparsecs away from the sun. It is the closest system to alioth the capital of the alliance. The first two later named taphao thong and taphao kaew are believed to orbit the star.

Vy ursae majoris facts. It s located 1 3 degrees south of r uma. Vy ursae majoris is a carbon star type star.

Preliminary version sky2000 master. It has an apparent magnitude that varies from 6 5 to 9 6 and its absolute magnitude is 9 4. Vy ursae majoris is not part of the ursa major constellation outline but is within the borders of the constellation.

Ux ursae majoris was first discovered to be variable in 1933 by s. Mizar hay zeta ursae majoris ζ uma ζ ursae majoris là một hệ 4 sao nằm ở vị trí thứ hai tính từ cuối cánh tay đòn của chòm sao đại hùng tên gọi mizar có nguồn gốc từ tiếng ả rập ميزر mi zar nghĩa là cạp quần váy hay đai. Vy ursae majoris is a semi regular variable carbon star c6 with a magnitude range of 5 8 to 6 4 over a period of 120 days.

A carbon star is a late type giant star similar to a red giant or. Based on the spectral type c5ii of the star the star s colour is carbon red. Trong tiếng trung nó được gọi là 開陽 sao khai dương.

It s circumpolar and high in the sky right now so it can make for an uncomfortable observation for some telescope users. I iii catalogues and names. Combined general catalogue of variable stars vol.

To get started try for vy ursae majoris. 78 ursae majoris is an alliance system in the core systems within the inner orion spur. Vy uma hr 4195 hd 92839 sao 15274 bd 68 617.

With a relatively constant light curve interrupted by eclipse induced drops in magnitude ux uma was orginally thought to be an algol type eclipsing variable ux uma s earliest claim to fame was its ultra short orbital period of 0 1967 days or 4 7 hours. Vy uma is a carbon star with a magnitude range of 6 0 to 6 6 in an irregular period. 47 ursae majoris abbreviated 47 uma formally named chalawan ˈ tʃ ɑː l ə w ə n is a yellow dwarf star approximately 46 light years from earth in the constellation of ursa major as of 2011 three extrasolar planets designated 47 ursae majoris b c and d.

1 system layout 2 minor factions 3 timeline 4 references 78 ursae majoris a class f star 78 ursae majoris a 1 landfall world high metal content treshchov gateway surface port seddon gateway orbis starport 78 ursae majoris a 1 a.

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