▁similar ▁or bits , ▁which ▁result ▁in ▁them ▁being ▁most ▁easily ▁visible ▁from ▁the ▁southern ▁hem is phere , ▁between ▁August ▁and ▁April . ▁Kre utz ▁s ung raz ers ▁appearing ▁between ▁May ▁and ▁July ▁may ▁come ▁and ▁go ▁un seen , ▁as ▁they ▁approach ▁from ▁directly ▁behind ▁the ▁Sun ▁as ▁seen ▁from ▁Earth ; ▁the ▁only ▁previous ▁Kre utz ▁S ung ra zer ▁seen ▁during ▁these ▁months ▁was ▁the ▁Eclipse ▁Com et ▁of ▁ 1 8 8 2 , ▁which ▁was ▁only ▁observed ▁once , ▁during ▁a ▁total ▁solar ▁eclipse . ▁ ▁Before ▁White – O rt iz – B ole l li , ▁studies ▁had ▁divided ▁the ▁Kre utz ▁S ung raz ers ▁into ▁two ▁sub - groups , ▁origin ating ▁from ▁fragment ations ▁at ▁different ▁or bits , ▁but ▁White - O rt iz - B ole l li ▁seemed ▁to ▁be ▁a ▁member ▁of ▁neither . ▁Studies ▁showed ▁that ▁it ▁probably ▁broke ▁away ▁from ▁the ▁com et ▁that ▁spawn ed ▁Sub group ▁II , ▁before ▁the ▁main ▁fragment ation , ▁and ▁it ▁was ▁class ed ▁as ▁the ▁first ▁( and ▁so ▁far ▁only ) ▁member ▁of ▁Sub group ▁II a . ▁ ▁Having ▁an ▁observation ▁arc ▁of ▁only ▁ 1 4 ▁days ▁with ▁a ▁likely ▁assumed ▁near ▁peri hel ion ▁orb ital ▁ecc ent ric ity ▁of ▁ 1 . 0 ▁( ep och ▁ 1 9 7 0 - May - 1 4 ), ▁it ▁is ▁unknown ▁if ▁this ▁par abol ic ▁com et ▁will ▁be ▁e ject