The Astrology of Space - Matrix Software

The Astrology of Space
nuclear or central bulge (decreasing from Sa to Sc)
and the relative strength of the arms (increasing from
Sa to Sc). Elliptical galaxies have a smooth structure
from a bright center out to indefinite edges and they
differ only in ellipticity, from round (E0) to a 3:1 axis
ratio (E7). Spiral galaxies show their typical spiral
arms or whorls emerging either directly from a bright
round nucleus (ordinary spirals) or at the ends of a
diametrical bar (barred spirals). Irregular galaxies are
either of the Magellanic Cloud type or chaotic, and
difficult to classify in the Hubble method. This method
was later revised to include the SO Or lenticular type
of galaxy, which shares the smooth structure of the
ellipticals, but has a definite, nucleus, occasional
interstellar matter, and luminosity similar to the
spirals. There are also two varieties of the barred
spiral, the classical S-shaped spirals (s) and the
ringed type (r) in which the arms start at the rim of an
inner ring. Transition types exist between all the main
types. There also appear to be large numbers of
"dwarf galaxies" that are small, have low surface
brightness, and are difficult to detect. Dwarfs exist
only as ellipticals or Magellanic irregulars. The
beautiful spirals appear to only occur among the giant
galaxies.
Galaxies Table
## Zodiac Latitude Name
G 26°Ar54'52 +33°55'48 NGC 205
Local Group, Andromeda, A8
G 18°Ar49'51 +36°39'31 NGC 221
Local Group, M.32, And.,G3
G 27°Ar09'25 +33°20'59 NGC 224, M.31
Local Group, G5, And.
G 01°Ar26'55 -23°36'05 NGC 247,
Sculptor Group, Cetus, Em
G 08°Ar55'46 -21°09'08 Cluster A
400 galaxies
G 29°Ar25'39 +23°54'05 Pisces cluster
100 galaxies
G 27°Ta37'33 +41°40'45 Maffei I
270