Sistema Solar

Neptune’s little moons are the exposed guts of worlds Triton destroyed

Using JWST's NIRSpec spectrograph, a team led by M. Ryleigh Davis has detected clay minerals on Neptune's small moons Larissa and Galatea and in its rings — the first such detection on any outer solar system body beyond Jupiter. Because these phyllosilicates form only through alteration by liquid water, they must have originated deep inside larger, warmer moons that were destroyed when Triton was captured. Neptune's inner moons may therefore be the exposed interiors of ancient icy worlds. Published in Science Advances.

Nuevos

Milky Way’s fastest star orbits our supermassive black hole so closely it feels its spin

Astronomers using ESO's Very Large Telescope Interferometer have discovered S301, the fastest known star in the Milky Way, orbiting the supermassive black hole Sagittarius A* at 25,000 km/s — over 8% of the speed of light — and completing an orbit in just 8.7 years. Published in Nature by the GRAVITY+ collaboration, the star passes close enough to feel the black hole dragging spacetime, making it the first star that could directly measure a supermassive black hole's spin — a key test of Einstein's general relativity.

A cosmic particle accelerator and the halo it built: the case for Cygnus X-3 behind the Cygnus Bubble

A team led by Zhaodong Shi (University of Science and Technology of China) has proposed that the microquasar Cygnus X-3 — recently confirmed as the Milky Way's first "super-PeVatron" — is the cosmic accelerator powering the mysterious Cygnus Bubble, a gamma-ray structure thousands of light-years across. Their model reproduces both the bubble's brightness and shape if Cygnus X-3 channels just 1-3% of its power into particle acceleration. Published in The Astrophysical Journal Letters.

Cosmología

Exploración Espacial

Coreanos fotografiaron el sitio exacto en la Luna donde SpaceX contaminó con chatarra espacial, Musk guarda silencio

El orbitador lunar surcoreano Danuri ha capturado imágenes del antes y el después del cráter que una etapa superior de un Falcon 9 de SpaceX excavó al estrellarse contra la Luna el 5 de agosto de 2026. El cuerpo del cohete, de 4.000 kg, impactó a unos 8.690 km/h formando un cráter de hasta 27 metros. La agencia coreana KARI realizó ocho pasadas sobre el sitio, y desde España se habría captado el video de la eyección.
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Radioastronomía

Vida extraterrestre

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    El SETI Institute confirma que el cometa interestelar 3I/Atlas no porta tecnología alienígena

    El SETI Institute rastreó cerca de 74 millones de señales de radio provenientes del cometa interestelar 3I/Atlas y no encontró ninguna tecno-firma. El objeto, estimado entre 440 m y 5.6 km y posiblemente de 11 mil millones de años, es completamente natural.

    Física

    The early universe’s giant galaxies are hiding their true weight in small stars

    Using the James Webb Space Telescope, an international team led by Leiden University has, for the first time, reliably measured the mix of tiny and giant stars in nine massive early galaxies — finding their stellar populations are bottom-heavy, packed with far more low-mass stars than galaxies like the Milky Way. As a result, these cosmic titans may be much more massive than thought; one, formed less than 1.5 billion years after the Big Bang, may be up to four times heavier than previous estimates. Published in Nature Astronomy.

    Un grumo invisible de materia oscura podría haber curvado el chorro de un blázar emisor de neutrinos

    Astrónomos liderados por Silke Britzen (Instituto Max Planck de Radioastronomía) han encontrado indicios de que un grumo invisible de materia oscura curvó gravitacionalmente el chorro del blázar PKS 2233-148, una de las pocas fuentes candidatas de neutrinos cósmicos. Combinando radio, rayos gamma y rayos X, detectaron un desplazamiento súbito del chorro junto a un destello ultrarrápido que podría ser la primera firma de subestructura de materia oscura detectada de esta forma. Publicado en MNRAS.

    Turning the cosmic web into a detector: first limits set on dark matter decaying into gravitons

    A team led by David Dunsky (New York University) has set the first observational limits on the exotic possibility that dark matter decays into gravitons. Using the magnetic fields of the cosmic web as a natural detector, gravitons crossing these filaments could convert into gamma-ray photons via the Gertsenshtein effect — a faint glow absent from Fermi-LAT data, which constrains the decay rate across a wide range of dark matter masses. Published in Physical Review D.

    Galaxy spins retain a measurable fingerprint from the universe’s first moments

    A team led by Ming-Jie Sheng (Xiamen University) has found the clearest evidence yet that galaxy rotation carries an imprint from the universe's first moments. By reconstructing the primordial distribution of matter with the ELUCID project and comparing it to measured galaxy spins, they detected the signature of primordial tidal torques with high statistical confidence — strongest in the gas of massive elliptical galaxies — confirming a decades-old prediction and opening a possible new probe of cosmic neutrinos.

    A minority of «leaky» galaxies may have reionized the early universe, JWST spectra suggest

    A team led by Emma Giovinazzo (University of Geneva) has analyzed JWST/NIRSpec spectra of 1,428 galaxies at redshift 5 to 10 and found that cosmic reionization may have been driven by a minority of "strong leaker" galaxies. Though only about 20% of galaxies let more than 10% of their ionizing radiation escape, these produced roughly 87% of the photons that reached the intergalactic medium — enough to account for nearly all reionization by z ≈ 5.8.

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