Theory of 16 stars as their volume total in reference to observing sun rise and sun set types of star set and star rise in relation to other star systems
and their star rise and star set as the number of such interactions increases to a way to which there are 16 stars related to each other as
connected by the star set and star rise on each of the stars planets and their horizons.
by Henryk Szubinski
Observations of stars on the horizons of their interactive star set or rise as related to many stars that do this throughout the day but also in the night as related
to our sun and other stars and their horizons that do this with the sun and other horizons so that even these stars have many sun rise and set of the many
star sets and star rise.
by Henryk Szubinski
from Wikipedia
date, 07,09,2016
time, 14:22
Procyon (BrE /ˈproʊsi.ɒn/;[12] pro-see-on), also designated Alpha Canis Minoris (α Canis Minoris, abbreviated Alpha CMi, α CMi), is the brightest star in the constellation ofCanis Minor. To the naked eye, it appears to be a single star, the eighth brightest in the night sky with a visual apparent magnitude of 0.34.[3] It is a binary star system, consisting of a white main-sequence star of spectral type F5 IV–V, named Procyon A, and a faint white dwarf companion of spectral type DQZ,[5] named Procyon B.
The reason for its brightness is not its intrinsic luminosity but its relative closeness to the Sun. As determined by the European Space Agency Hipparcos astrometry satellite,[1][13] it lies at a distance of just 11.46 light-years (3.51 parsecs),[2] and is therefore one of Earth's nearest stellar neighbours. Its closest neighboring star is Luyten's Star, about 1.12 ly (0.34 pc) away, and the latter would appear as a visual magnitude 2.7 star in the night sky of a hypothetical planet orbiting Procyon.[14]
to our sun and other stars and their horizons that do this with the sun and other horizons so that even these stars have many sun rise and set of the many
star sets and star rise.
by Henryk Szubinski
from Wikipedia
date, 07,09,2016
time, 14:22
Procyon (BrE /ˈproʊsi.ɒn/;[12] pro-see-on), also designated Alpha Canis Minoris (α Canis Minoris, abbreviated Alpha CMi, α CMi), is the brightest star in the constellation ofCanis Minor. To the naked eye, it appears to be a single star, the eighth brightest in the night sky with a visual apparent magnitude of 0.34.[3] It is a binary star system, consisting of a white main-sequence star of spectral type F5 IV–V, named Procyon A, and a faint white dwarf companion of spectral type DQZ,[5] named Procyon B.
The reason for its brightness is not its intrinsic luminosity but its relative closeness to the Sun. As determined by the European Space Agency Hipparcos astrometry satellite,[1][13] it lies at a distance of just 11.46 light-years (3.51 parsecs),[2] and is therefore one of Earth's nearest stellar neighbours. Its closest neighboring star is Luyten's Star, about 1.12 ly (0.34 pc) away, and the latter would appear as a visual magnitude 2.7 star in the night sky of a hypothetical planet orbiting Procyon.[14]
By knowing the 16 stars ,the angle may be related to 1 degree for example so that the whole universe of the billions and trillions of stars are related to this degree and any system may be found as volume relations of those stars with the gravity of each having ,for example 16 gravity units, depending on how many multiple or decimal sets of the 16 g are used.