-
Low M**** (Latin
Missa Privata) is a
Tridentine M**** defined officially in the Code of
Rubrics included in the 1962
edition of the
Roman Missal as a M****...
-
classification by
m**** (high, intermediate,
low)
refers to the
optically visible donor, not to the
compact X-ray
emitting accretor.
Low-
m**** X-ray binaries...
- : §1
After the hydrogen-fusing
period of a main-sequence star of
low or
intermediate m**** ends, such a star will
expand to a red
giant and fuse
helium to...
- be
typical of the
Solar System's
rocky matter, and a
m**** approximately 2.25
times its
current m****.
Early in the
Solar System's history,
Mercury may have...
- was very red and enigmatic,
showing none of the
features expected of a
low-
m**** red dwarf. It
became clear that GD 165B
would need to be
classified as...
- none has yet had time to
evolve to this
point and be observed.)
Low-
m**** stars with a
m**** below about 1.8–2.2 M☉ (depending on composition) do
enter the...
- surprising,
because current theories of
planetary formation suggest that
low-
m**** planets should have
their orbital eccentricity circularized by gravitational...
- The
Tridentine M****, also
known as the
Traditional Latin M**** or the
Traditional Rite, is the
liturgy in the
Roman Missal of the
Catholic Church codified...
- environment. Accordingly,
astronomers often group stars by
their m****: Very
low m**** stars, with m****es
below 0.5 M☉, are
fully convective and distribute...
-
parts of the
M**** to be sung, and the use of incense. It is also
called High
M**** or
Solemn High
M****.
These terms distinguish it from a
Low M**** and Missa...