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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Astronomers using NASA's Hubble Space Telescope have identified a faint galaxy called CDG-2, located 300 million light-years away in the Perseus cluster, that consists almost entirely of dark matter. The discovery relied on detecting four globular clusters rather than the galaxy's dim stars. This finding highlights the role of dark matter in low-surface-brightness galaxies.

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Astronomers have uncovered evidence that a black hole and neutron star merged while following an unusual oval-shaped orbit, challenging expectations of circular paths in such events. The discovery comes from a reanalysis of gravitational wave data from the event known as GW200105. This finding suggests the system formed in a dynamic stellar environment.

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