parshyaa said:
Sorry for this thread ,but he said that time of free fall does depends on mass , if any budy proved this then he will get a nobel prize and scientists are buisy to crack this. Suppose they have proved that yes it does depends on mass , then what will happen to the formula for time t, what is wrong in arguing that inertial mass and gravitational mass can be different[then this argument will raise a question how can a object have two mass] , oh god I am confused and making others too
@parshyaa (and Sophiecentaur) and whoever else...Maybe I can clarify a bit...Hopefully. It seems that the confusion is arising because there seems to be some confusion about
which mass, (central mass or orbiting mass) you guys are referring to when commenting (it needs to be clarified) AND also because someone (Turtlemeister) used a "free -fall" equation based upon Kepler's 3rd law of ORBITAL motion...(which, BTW, is mass dependent) .. Let me explain>..and maybe it will help...maybe..LOL...It will require you to look at the equation briefly. OK, don't stop reading yet, this will be simple, not like my previous post.
Kepler's Law states (as mentioned by sophiecentaur) that an orbital planet sweeps out equal areas in equal times. What this means is that the orbital
period, T, squared divided by the orbital
Radius (or semi-major axis) CUBED is equal to a
CONSTANT for ALL planets revolving around the CENTRAL MASS. Yes, amazingly the ratio of the orbital period squared to the orbital radius cubed is
THE SAME value for
ANY planet or asteroid or anything orbiting the sun.... Now what Sopie
didn't mention is that this
CONSTANT is equal to
4 (pi)^2 / GM...where M is the large Mass of the central body...(and G is the "gravitational constant".) This "Kepler" constant is dependent only on the central mass, say the sun for example,
as long as the orbiting planets (or whatever) have "negligible" mass compared to the sun. As soon as a planet's mass becomes appreciable, then its mass, m, must be included in the calculation.
This Kepler orbital equation of motion can be manipulated to arrive at free-fall motion, (to which Turtlemeister alluded)...but this is not typical... This no doubt caused some confusion...
The amazing genius of Kepler's equation is that it is applicable for
all bodies orbiting around the same central mass. For example,,,ALL satellites orbiting Earth must follow the same Kepler equation (except now using mass of Earth as big M) . IOW, all satellites with the same orbital radius must have the same orbital period...(and even satellites in elliptical orbits have the same orbital period provided we substitute its semi-major axis for radius, R.) This is because the formula depends only upon the mass of Earth and the satellites have "negligible" mass compared to that of earth.
Pres. Eisenhower in 1957, being greatly troubled, for example, when Russia sent the first orbiting satellite (Sputnik) over America, asked US scientists," How can we determine how big (how massive) this Russian satellite is?" The response was , "We can't ... even if we know its orbital period and orbital radius".
Why ? Because the mass of the orbiting satellite does not enter into the equation of motion...only that of the central mass, (earth) ...providing that the satellite isn't a big bugger like that on the movie "Independence Day" ! (LOL).
NOW, having said all that, the above stuff really says almost nothing about "gravitational" verses "inertial" mass. To really enter into that discussion you must start with NEWTON's equations...which deal with INERTIAL mass via
F= ma...and combine it with gravitational Force equations like
F= GMm / R^2... which gives the force between two masses.
I think I've said enough for now. Clear as mud, right?
Pet Scan