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This scenario but we add a third object that will pass inside the Earth's orbit between the Earth and the small object and very fast to escape Earth's gravity and move away, so to momentarily exert a large gravitational force and to locally cancel (and more) Earth's gravitational pull to slow down the small object to about zero near ground level.
Tidal effects will be catastrophic so please don't do this to your home planet unless you really, really want to.
Yeah, with a Lagrange keyhole orbit past the Moon (which is what OP is asking about, not just plain escape velocity), you could park an Asteroid Belt asteroid in an orbit around the Earth. But it will be a high orbit. Not sure how low you could get it, I'm hoping a circular geostationary orbit is possible? But more likely something in the 300,000km range.
Low orbit is out of the question. Maaaybe you could park the asteroid in a highly elliptical orbit where the perigee is inside the atmosphere. The drag will circularize it if the asteroid is small enough. But not so small or weak that it burns up or breaks up before that happens. And not so big that drag takes too long and the orbit wobble makes it hit the surface. In a low Earth orbit you now only have 8km/s delta-v to deal with.
But to get the asteroid to gently touch the surface the way OP describes it, like some sort of skyhook? Is impossible short of a planet X or a rogue black hole passing even closer to the Earth than the Moon at the right moment. And whatever remains afterwards would be hard to call a surface: https://www.youtube.com/watch?v=kRlhlCWplqk