Maksim A. Burakhovich absolute time: since time is relative where on Earth time goes slower than in space since gravitational field slows time down, i guess we could designate absolute time as time at the center of mass of the heaviest object in the Universe that's not a black hole or where the difference in mass between that object and the litest black hole in terms of mass in the Universe is infinitesimal.
The Celsius scale is not absolute. It has no absolute value.
First, simplify the equation: absolute (3x-1) = absolute (x+5) absolute (2x) = absolute (6) absolute (x) = absolute (3) which really means plus or minus 3, or, (+/-3) Now you have x = +/- 3, so test out x = 3 and x = -3. Test out x = 3: absolute (3*3-1) = absolute (3+5) absolute (9-1) = absolute (8) ---> absolute 8 = absolute 8 --> 8=8 which is correct! Now test x = -3 absolute (3*(-3)-1) = absolute (-3+5) ---> absolute (-9-1) = absolute (2) absolute (-10) = absolute 2 ---> 10 = 2 Since 10 does not equal 2, this is not a correct answer. Therefore x = 3.
Absolute 4 is 4. The question is now "what is 4-8b absolute = 12. There is an "absolute" here operating on nothing. This is still true if you mean absolute(4-8b) absolute =12 so the question cannot be interpreted.
The age of absolute
Fomalhaut b was created in 2008.
Fomalhaut appears to be a bright white star to the naked eye.
Fomalhaut is a white main sequence star located in the constellation Piscis Austrinus.
The distance of Fomalhaut from the solar system is listed as 25.1 light-years.That's something like 1.6 million times the distance from the earth to the sun !
Fomalhaut has a declination of almost -30° (30° south), so it can be seen - at least in theory - at latitude 60° north, or anywhere south of that.
An absolute unit is a unit which can be exactly defined in terms of mass, length, or time.
It is the smallest particle
Mass and age.
not very heavy
The absolute mass of an electron is approximately 9.109 x 10^-31 kilograms.
Aldebaran (the star 4 spring)Regulus (summer)Antares(autumn)Fomalhaut (winter)
the larger the mass of the star, the more luminous it is.