Roman space telescope could reveal hidden neutron stars

NASA's upcoming Nancy Grace Roman Space Telescope may detect dozens of isolated neutron stars in the Milky Way through gravitational microlensing. A new study shows the observatory could measure the masses of these otherwise invisible objects. Researchers expect the mission to provide the first large sample of such stars detected solely by their gravitational effects.

Astronomers estimate the Milky Way contains tens to hundreds of millions of neutron stars, yet only a few thousand have been identified, mostly as pulsars. Most remain hidden because they emit little or no detectable light. The Roman telescope will repeatedly observe millions of stars in the galactic bulge, allowing it to spot the subtle brightening and positional shifts caused when a neutron star passes in front of a distant background star.

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NASA’s Nancy Grace Roman Space Telescope is expected to discover around 100000 previously unknown exoplanets. This would mark a major increase from the nearly 6300 worlds identified so far. The mission will survey distant regions of the Milky Way using transit and microlensing methods.

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NASA has set August 30, 2026, as the launch date for the Nancy Grace Roman Space Telescope, moving the schedule up by eight months from earlier plans.

A theoretical study proposes that collapsing massive stars may form gravastars rather than black holes by creating miniature universes inside themselves. The model offers the first dynamic explanation for how these exotic objects could arise from ordinary stellar matter.

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