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How ripples in space-time can reveal new exoplanets | News.gg

Wednesday, November 11, 2026Coverage from every side, on News.ggInternational Edition

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Published 21 hours ago · Phys.org · Updated 3 hours ago

Off the radar: covered mostly by the center

Space boffin discovers Earth's new 'mini-moon' after it was sucked in by gravity

Side-by-Side Framing

The LISA (Laser Interferometer Space Antenna) observatory, now in development, will detect gravitational waves, the tiny ripples in space-time caused by orbiting masses.
Now two studies led by NASA astrophysicists show in new detail how LISA could reveal a new and unique population of exoplanets—worlds beyond our solar system—throughout our galaxy.

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Phys.orgFactualityFactuality is a Premium featureHow reliably the outlets covering this story report facts, based on their track record of accuracy and corrections.

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How ripples in space-time can reveal new exoplanets

The LISA (Laser Interferometer Space Antenna) observatory, now in development, will detect gravitational waves, the tiny ripples in space-time caused by orbiting masses. Now two studies led by NASA astrophysicists show in new detail how LISA could reveal a new and unique population of exoplanets—worlds beyond our solar system—throughout our galaxy.

Nov 11, 2026, 12:40 AM UTC

Read full article at Phys.org

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1 Article

Phys.orgFactualityCenter
How ripples in space-time can reveal new exoplanets
The LISA (Laser Interferometer Space Antenna) observatory, now in development, will detect gravitational waves, the tiny ripples in space-time caused by orbiting masses. Now two studies led by NASA astrophysicists show in new detail how LISA could reveal a new and unique population of exoplanets—worlds beyond our solar system—throughout our galaxy.
21 hours ago · phys.org · You are reading this one

Coverage Details

Total News Sources: 8
Leaning Left: 2
Leaning Right: 1
Center: 13
Last Updated: 3 hours ago
Bias Distribution: 81% Center

Bias Distribution

• 81% of the sources are Center

L 13%

C 81%

Phys.orgCenter · phys.org

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