Category Astronomy/Space

Blood proteins may flag disability risk years before loss of independence

Towards early disability prediction with blood protein biomarkers
Researchers identified two blood proteins—beta-2-microglobulin (B2M) and cystatin C—that predict future disability in community-dwelling adults aged 85 years and older. The findings, validated in independent Japanese and Italian aging cohorts, suggest that blood-based biomarkers could support earlier identification of older adults at risk of losing independence and guide timely preventive interventions. Credit: Dr. Yusuke Osawa from Keio University, Japan

Japan has one of the world’s fastest-aging populations, but maintaining independence into very old age remains a growing public health challenge...

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ALMA uncovers sulfur for the first time around a rare class of supergiant star

Astronomers have discovered a chemically rich collection of sulfur-bearing molecules surrounding the rare massive star HD 87643. The observations include the first detection of sulfur monoxide and sulfur dioxide around a B[e] supergiant. The paper was published in The Astrophysical Journal Letters on July 1.

Rare and old
B[e] supergiants, or sgB[e], are rare, evolved massive stars that have moved past their main hydrogen-burning phase. They are notable for distinctive emission lines—hence the “[e]” in their name—including rare “forbidden” lines produced by the surrounding gas and dust, along with an infrared glow far more intense than that of ordinary B-type stars.

As these stars approach the final stages of their lives, they shed enormous amounts of material, building up mes...

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Interplanetary spacecraft capture a coronal mass ejection component hidden from Earth

Interplanetary spacecraft capture a coronal mass ejection component hidden from Earth
Extreme ultraviolet (EUV) and coronagraph observations of the solar disk and corona highlighting the extended filament that produced the complex CME. Credit: Science Advances (2026). DOI: 10.1126/sciadv.aed9960

During a coronal mass ejection (CME), the sun hurls billions of tons of magnetized plasma into space. These eruptions are among the most powerful events in the solar system, and when they are aimed toward Earth, they can seriously threaten the satellites and power grids we depend on. For now, it remains notoriously difficult to predict how these eruptions evolve over time—and, in turn, whether they might be heading toward us.

Taking observations from an extensive network of spacecraft across the solar system, a team led by Adrienn Luspay-Kuti at Johns Hopkins University h...

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Radio telescopes help scientists map molecules in space and uncover where and how stars form

The Orion Nebula with pink and purple gas and brown dust.
The Orion Nebula, captured in visible light by the Hubble Space Telescope. NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team

You may have heard the phrase “we are made of star-stuff.” This statement by the astronomer Carl Sagan refers to the fact that elements heavier than hydrogen and helium were forged in the centers of the first stars. But how does this star-stuff evolve into the chemistry of rocks, plants and people?

As an astrochemist and radio astronomer, I study the places in the universe where stars are born as interstellar laboratories. I’m interested in how simple ingredients come together to form bigger and bigger molecules, including those that are building blocks of life...

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