HD 33579
HD 33579 is a white/yellow hypergiant and one of the brightest stars in the Large Magellanic Cloud (LMC). It is a suspected variable star. HD 33579 lies in a part of the Hertzsprung–Russell diagram referred to as the Yellow Evolutionary Void because stars with that combination of luminosity and temperature are extremely unstable. They either expand to become cooler or shed their outer layers completely to become hotter. Yet HD 33579 is relatively stable, hardly even variable. This is thought to be due to its higher mass compared to most stars with similar temperature and luminosity.
Link from a Wikipage to another Wikipage
primaryTopic
HD 33579
HD 33579 is a white/yellow hypergiant and one of the brightest stars in the Large Magellanic Cloud (LMC). It is a suspected variable star. HD 33579 lies in a part of the Hertzsprung–Russell diagram referred to as the Yellow Evolutionary Void because stars with that combination of luminosity and temperature are extremely unstable. They either expand to become cooler or shed their outer layers completely to become hotter. Yet HD 33579 is relatively stable, hardly even variable. This is thought to be due to its higher mass compared to most stars with similar temperature and luminosity.
has abstract
HD 33579 is a white/yellow hyp ...... a possible period of 27 days.
@en
HD 33579 — біло-жовтий гіпергі ...... ся, що зоря може бути змінною.
@uk
HD 33579是大麥哲倫星系內的一顆恆星。 它是一顆白/黃 ...... 上，雖然它的光譜類型是A3，也意味著它也被描述為白特超巨星。
@zh
Wikipage page ID
35,862,340
page length (characters) of wiki page
Wikipage revision ID
1,016,001,082
Link from a Wikipage to another Wikipage
absmag v
−9.57
@en
appmag v
+9.22
@en
b-v
+0.14
@en
class
A3Ia+
@en
constell
dist ly
~165,000
@en
dist pc
~50,000
@en
epoch
luminosity
p error
parallax
prop mo dec
−0.46
@en
prop mo ra
radial v
2.55959e+2
temperature
u-b
−0.29
@en
variable
wikiPageUsesTemplate
subject
hypernym
comment
HD 33579 is a white/yellow hyp ...... ar temperature and luminosity.
@en
HD 33579 — біло-жовтий гіпергі ...... ся, що зоря може бути змінною.
@uk
HD 33579是大麥哲倫星系內的一顆恆星。 它是一顆白/黃 ...... 上，雖然它的光譜類型是A3，也意味著它也被描述為白特超巨星。
@zh
label
HD 33579
@en
HD 33579
@sv
HD 33579
@uk
HD 33579
@zh
wasDerivedFrom
isPrimaryTopicOf
name
HD 33579
@en