Page 5: Research news on Optical astronomy

Optical astronomy is the research area focused on observing and analyzing electromagnetic radiation in the optical band, typically encompassing near-ultraviolet, visible, and near-infrared wavelengths accessible to ground- and space-based telescopes using optical elements and detectors. It employs instruments such as imaging cameras, spectrographs, and polarimeters on refracting or reflecting telescopes to study the photometric, spectroscopic, and polarimetric properties of astronomical sources. The field addresses topics including stellar and galactic structure, interstellar medium characterization, planetary systems, and cosmological parameters, and it relies on advanced techniques in adaptive optics, precision calibration, and data reduction to mitigate atmospheric and instrumental effects.

ESA's new asteroid hunter opens its eye to the sky

The European Space Agency's (ESA) newest planetary defender has opened its "eye" to the cosmos for the first time. The Flyeye telescope's 'first light' marks the beginning of a new chapter in how we scan the skies for new ...

Turning down starlight to spot new exoplanets

Researchers have developed a new coronagraph—an optical device that blocks out light from a bright source—that could make it possible to see distant exoplanets obscured by light from their parent stars. The new device could ...

Preparing for the greatest cosmic movie ever made

High up on the top of Cerro Pachón in northern Chile, NSF–DOE Vera C. Rubin Observatory is nearing completion. At the heart of the facility, a pivotal moment in the project's scientific adventure is unfolding. After more ...

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