Earth has a Schwarzschild radius of about 3 mm.
This means things at geostationary orbital distance have a time dilation of about
$$\sqrt{1-\frac{9 mm}{35786 km}}$$
or one part in $10^{-10}$ roughly. (if they are actually orbiting this value changes slightly, as does the rotation of the Earth)
This also lines up with the length contraction factor.
When the Earth disappears "instantly", a gravitational wave of that magnitude is going to be produced. How much energy is that?
Well, 1 solar mass converted to gravitational waves and sent over 1.4 billion light years produced a $10^{-20}$ amplitude wave (LIGO observation). The energy in a gravitational wave is proprotional to amplutide squared.
So, per meter squared, the LIGO observation would carry:
(1 solar mass * c^2) / (1.4 billion light years*2)^2 / 4 pi * 1 m^2
2 * $10^{-5}$ J (apparently it was 1 solar mass of matter converted into a gravitational wave at a distance of 1.4 billion light years).
The gravitational wave from the Earth disappearing is going to be ${10^{10}}^{2}$ stronger than that, or 2*$10^{15}$ J. This is an insane amount of energy; however, very little of it actually deposits on normal matter.
Suppose we are 1 Jupiter-radius away from Jupiter instead.
Jupiter has a Schwarzschild radius of 2.2 m. Titan has an average orbit of 1,221,850 km. Then the gravitational wave would carry 500 times as much Energy.
The question becomes how well does it convert over to normal matter? Will it occur fast enough to disrupt an atomic nucleus?
The compression effect on molecular-level matter will only involve modest pressures. But the compression effect will occur all the way down the length scales, and I suspect it requires lots more pressure to compress a nucleus.
But back up a second. We ripped the planet from our universe. One could argue that would involve forming an event horizon around the planet and making it disappear.
I mean, photons not coming from an area is the definition of event horizon. Stuff an event horizon somewhere, and you warp space. The volume we need to swallow is the planet. So, black hole the size of the planet in effect blinks in then poofs?
If we are 10 planet-radius away, and the event horizon forms tightly around the planet then disappears, this would generate two gravitational waves of impressive magnitude.
$$\sqrt{1 - \frac{1 r}{10 r}}$$
gives us a amplitude of 0.05. The energy carried by this wave is about 10^17 times greater than the ones we are describing above.
In effect, all matter would suddenly feel stretched by 5%, then compressed by 5%. This would occur all the way down to the molecules, quarks and nuclei. I'd be worried about fission events from this happening suddenly, let alone the amoung of energy released by compressing "incompressible" solids by 5%.
Compressing water by 5% would take 0.1 GPa, so we could estimate the effect would be akin to a pressure wave of that magnitude over humans. And 0.4 GPa for iron.
This level of pressure in a conventional blast is enough to blow limbs off.
I cannot believe the compressibility of EM mediated molecule-scale solids is in the same universe as that for a nucleus or a proton. So I would be very worried about atomic disintegration...
Ignoring that, matter slows down gravitational waves. The effect is extremely tiny, but we could use that to estimate how much impulse this would provide and how much energy deposited. I cannot find the correct equations for this case.
Calculating what exactly happens is going to be quite tricky. For a planet-sized event horizon, the effect will be explosive at "molecular" scales, blowing objects apart. At atomic scales, I don't know (will it cause fission?). At macroscopic scales, I don't know (will it impart a large radial impuse from the matter slowing the gravitational wave down?).
There is plenty of energy to work with. The kind of effect that energy density and flux could cause seem unbounded.
The above also neglects the power; how long the teleport takes determines the power the wave carries (how "sharp" it is, not just how much energy it carries).