description DX Cancri Overview
DX Cancri is a nearby red dwarf in the constellation Cancer, approximately 12 light-years from Earth. It is an M-type main-sequence star with only a small fraction of the Sun's mass and luminosity, placing it near the lower end of stars capable of sustained hydrogen fusion. DX Cancri is also classified as a flare star because magnetic activity can produce sudden increases in its brightness.
help DX Cancri FAQ
What is DX Cancri?
DX Cancri is a nearby red dwarf star in the constellation Cancer. It is an M-type main-sequence star approximately 12 light-years from Earth.
How does DX Cancri compare with the Sun?
DX Cancri has only a small fraction of the Sun's mass and luminosity. As a red dwarf, it is cooler, dimmer, and much smaller than the Sun.
Can DX Cancri be seen with the naked eye?
No, DX Cancri is far too faint for unaided human vision. Even though it is relatively close at about 12 light-years, red dwarfs emit very little visible light.
What type of star is DX Cancri?
DX Cancri is an M-type main-sequence star, commonly called a red dwarf. It lies near the lower mass and luminosity range for stars that sustain hydrogen fusion in their cores.
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