Liquid mirror telescopes use a thin layer of mercury and rotation to form a parabolic surface, making them cost-effective but limited in function.
A recent study proposes using a ferrofluid and electromagnets to improve liquid mirror telescopes, allowing for some degree of orientation and shape retention.
This method could be effective for space telescopes in environments with weaker gravity, such as on the Moon.
Although the feasibility has been explored, current electric circuitry needs improvement for practical implementation.