From: owner-ammf-digest@smoe.org (alt.music.moxy-fruvous digest) To: ammf-digest@smoe.org Subject: alt.music.moxy-fruvous digest V14 #11338 Reply-To: ammf@fruvous.com Sender: owner-ammf-digest@smoe.org Errors-To: owner-ammf-digest@smoe.org Precedence: bulk alt.music.moxy-fruvous digest Saturday, May 13 2023 Volume 14 : Number 11338 Today's Subjects: ----------------- Mom chews 46 lbs of fat away (brand-new diet) ["Eat yourself thin" Subject: Mom chews 46 lbs of fat away (brand-new diet) Mom chews 46 lbs of fat away (brand-new diet) http://cardiodefendx.life/mxs7CDsH0gCcYsVCt7Eip1kDs-jnXzrbi020PiE-OL3LfwiWfg http://cardiodefendx.life/9xzicrmfzUDoVbpqISMNQInndgKGyer3wetRRPTP61rq2jub-Q assive black hole (SMBH or sometimes SBH) is the largest type of black hole, with its mass being on the order of hundreds of thousands, or millions to billions of times the mass of the Sun (M?). Black holes are a class of astronomical objects that have undergone gravitational collapse, leaving behind spheroidal regions of space from which nothing can escape, not even light. Observational evidence indicates that almost every large galaxy has a supermassive black hole at its center. For example, the Milky Way has a supermassive black hole in its Galactic Center, corresponding to the radio source Sagittarius A*. Accretion of interstellar gas onto supermassive black holes is the process responsible for powering active galactic nuclei (AGNs) and quasars. Two supermassive black holes have been directly imaged by the Event Horizon Telescope: the black hole in the giant elliptical galaxy Messier 87 and the black hole at the Milky Waybs center. Description Supermassive black holes are classically defined as black holes with a mass above 100,000 (105) solar masses (M?); some have masses of several billion M?. Supermassive black holes have physical properties that clearly distinguish them from lower-mass classifications. First, the tidal forces in the vicinity of the event horizon are significantly weaker for supermassive black holes. The tidal force on a body at a black hole's event horizon is inversely proportional to the square of the black hole's mass: a person at the event horizon of a 10 million M? black hole experiences about the same tidal force between their head and feet as a person on the surface of the earth. Unlike with stellar mass black holes, one would not experience significant tidal force until very deep into the black hole's eve ------------------------------ End of alt.music.moxy-fruvous digest V14 #11338 ***********************************************