SCP-037 appears to be a star approximately 5 cm (2 in) in diameter, with a luminosity of about 1*10-12 times that of our sun and a surface temperature of about 5000 K (determined by UBVRI analysis). The origin of SCP-037 is unknown, however, analysis suggests that it shares many properties in common with a typical main sequence star, other than its anomalously small size. It is theorized to have entered the Earth's magnetosphere via the North Magnetic Pole.

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