Puppycow
Penultimate Amazing
There are hypothetical creatures that COULD develop and live in the atmosphere of a gas giant like Jupiter. But a Brown Dwarf is probably even more massive, turbulent, and violent than a gas giant planet.
But, theoretically speaking, if a brown dwarf, after trillions upon trillions of years, wouldn't it be possible for life to form on the surface? I mean, after all of that time, even a brown dwarf would burn away a lot of it's mass. So maybe the surface of a black dwarf wouldn't have as strong a gravity as it did when it was even a brown dwarf.
No, because these are two very different things. A white dwarf never becomes a brown dwarf, but eventually it should become a black dwarf (there should not be any black dwarfs yet according to theory because the universe isn't old enough).
White dwarf (which becomes a black dwarf eventually)
A white dwarf, also called a degenerate dwarf, is a stellar remnant composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of the Sun, and its volume is comparable to that of the Earth. Its faint luminosity comes from the emission of stored thermal energy.[1]
. . .
White dwarfs are thought to be the final evolutionary state of all stars whose mass is not high enough to become a neutron star (including our Sun)—over 97% of the stars in the Milky Way.[5], §1. After the hydrogen–fusing lifetime of a main-sequence star of low or medium mass ends, it will expand to a red giant which fuses helium to carbon and oxygen in its core by the triple-alpha process. If a red giant has insufficient mass to generate the core temperatures required to fuse carbon, around 1 billion K, an inert mass of carbon and oxygen will build up at its center. After shedding its outer layers to form a planetary nebula, it will leave behind this core, which forms the remnant white dwarf.[6]
. . .
The material in a white dwarf no longer undergoes fusion reactions, so the star has no source of energy, nor is it supported by the heat generated by fusion against gravitational collapse. It is supported only by electron degeneracy pressure, causing it to be extremely dense.
. . .
A white dwarf is very hot when it is formed, but since it has no source of energy, it will gradually radiate away its energy and cool. This means that its radiation, which initially has a high color temperature, will lessen and redden with time. Over a very long time, a white dwarf will cool to temperatures at which it will no longer emit significant heat or light, and it will become a cold black dwarf.[6] However, the length of time it takes for a white dwarf to reach this state is calculated to be longer than the current age of the universe (approximately 13.8 billion years),[10] and since no white dwarf can be older than the age of the universe, it is thought that no black dwarfs yet exist.[1][5] The oldest white dwarfs still radiate at temperatures of a few thousand kelvins.
Brown dwarf
Brown dwarfs are substellar objects not massive enough to sustain hydrogen-1 fusion reactions in their cores, unlike main-sequence stars. They occupy the mass range between the heaviest gas giants and the lightest stars, with an upper limit around 75[1] to 80 Jupiter masses (MJ). Brown dwarfs heavier than about 13 MJ are thought to fuse deuterium and those above ~65 MJ, fuse lithium as well.[2] Brown dwarfs may be fully convective, with no layers or chemical differentiation by depth.[3]
The defining differences between a very-low-mass brown dwarf and a giant planet (~13 MJ) are currently being debated.[4] One school of thought is based on formation; the other, on the physics of the interior.[4]
Part of the debate concerns whether "brown dwarfs" must, by definition, have experienced fusion at some point in their history.
Stars are categorized by spectral class, with brown dwarfs being designated as types M, L, T, and Y.[4][5] Despite their name, brown dwarfs are of different colours.[4] Many brown dwarfs would likely appear magenta to the human eye,[4][6] or possibly orange/red.[7] Brown dwarfs are not very luminous at visible wavelengths.
In the picture above^^ a white dwarf would be about the same size as the earth. Much smaller than the brown dwarf in volume, but much heavier in mass. The mass is about the mass of the sun in that picture, crammed into the size of the earth. So it is extremely dense and has extremely strong gravity at the surface.