In a groundbreaking discovery, astronomers have identified TOI-1846 b, a super-Earth exoplanet located 154 light-years away.

The radial velocity method is best for finding exoplanets that are relatively nearby because it requires us to be able to ...

When astronomers first discovered exoplanets, they found massive ones orbiting large stars. The technology to detect smaller planets around low-mass, dim red dwarfs took time to develop. By the ...

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The significant challenge faced by underwater gravity matching navigation is the precise acquisition of velocity information for real-time Eötvös correction of marine gravimeters without emitting or ...

The shape parameters of Multiquadric Radial Basis Function (MQ-RBF) have great influence on its interpolation effect. In this paper, the selection method of shape parameters is studied, and the Random ...

Unlike the transit method and radial velocity method, the TTV technique is not subject to their specific observational challenges. Instead, it can indirectly detect the presence of a planet by simply ...

Astronomers have discovered thousands of exoplanets, some in the so-called habitable zone, Does that mean these planets could ...