Tag

Supernova

All articles tagged with #supernova

Betelgeuse’s Hidden Binary Holds Clues to Its Inevitable Supernova
science10 days ago

Betelgeuse’s Hidden Binary Holds Clues to Its Inevitable Supernova

Betelgeuse, the bright red supergiant in Orion, will someday explode as a supernova but likely not for about 100,000 years. New observations strengthen the case that Betelgeuse has a binary companion (Betelgeuse B) hidden in its glare, which could influence its evolution. When it finally collapses, the explosion will unleash an enormous energy burst—mostly in the form of neutrinos—and could heat and strip some mass from the companion, though both stars would largely survive. Earth’s distance would likely keep the event from being catastrophic, but many details about the system and timing remain uncertain.

X-ray shock breakout marks the death of a 30-solar-mass star, tracked for months
science13 days ago

X-ray shock breakout marks the death of a 30-solar-mass star, tracked for months

Astronomers detected an X-ray shock breakout signaling the core collapse of a star about 30 times the Sun’s mass, then watched the resulting broad-lined Type Ic supernova SN 2026gzf for nearly three months across multiple wavelengths. Located ~500 million light-years away, it produced no gamma-ray burst, suggesting jets were choked and the star likely left a black hole, providing a rare, detailed look at the end stages of massive-star evolution.

Global telescope network captures early shock-breakout of a colossal stellar explosion
space-and-astronomy19 days ago

Global telescope network captures early shock-breakout of a colossal stellar explosion

Astronomers worldwide recorded the first moments of a 500‑million‑light‑year‑distant Type Ic broad‑lined supernova from a Wolf–Rayet progenitor, catching the faint X-ray shock breakout and mapping the star’s pre‑explosion surroundings; the event showed jets but no observed gamma‑ray burst, suggesting a possible choking of the jet, with Rubin Observatory and other facilities continuing long‑term follow‑up observations.

Global telescope network captures earliest moments of a distant supernova in unprecedented detail
space20 days ago

Global telescope network captures earliest moments of a distant supernova in unprecedented detail

A network of ground- and space-based telescopes, including the Vera C. Rubin Observatory, captured the first moments and subsequent evolution of a Type Ic broad‑lined supernova roughly 500 million light-years away. The observations detail the shock breakout and early light with unprecedented clarity, and follow-up studies found no accompanying gamma-ray bursts, suggesting a possible choked jet. Researchers mapped the star’s pre‑explosion environment around a Wolf‑Rayet progenitor, and Rubin’s continued, high-cadence monitoring will provide long-term data on this event and many future supernovas.

Faint X-ray shock breakout reveals a new path for massive-star deaths (SN 2026gzf)
space20 days ago

Faint X-ray shock breakout reveals a new path for massive-star deaths (SN 2026gzf)

Astronomers tracked SN 2026gzf from its faint X-ray shock breakout to its early light across multiple wavelengths, revealing a broad-lined Type Ic explosion from a Wolf‑Rayet star about 500 million light-years away that did not produce a gamma-ray burst. The rapid, multi-instrument follow-up mapped the explosion and its interaction with surrounding material, suggesting diverse pathways to such energetic deaths beyond GRB jets and shedding light on the star’s final years.

Rare double-supernova binary reveals history of two massive stars
science1 month ago

Rare double-supernova binary reveals history of two massive stars

Scientists report evidence that two massive stars in a binary system both exploded as supernovas, creating the Jellyfish Nebula (IC 443) and a nearby nebula (G189.6+3.3). Based on more than a decade of NASA’s Fermi observations, the progenitors were roughly 15–25 and at least 20 solar masses; their explosions occurred tens of thousands of years apart, and the remnants are likely neutron stars. This rare system provides direct clues to how massive binaries evolve and end their lives.

First known binary-star pair where both stars exploded as supernovae
space1 month ago

First known binary-star pair where both stars exploded as supernovae

Astronomers analyzing 16+ years of multiwavelength data (including NASA’s Fermi gamma-ray observations) identify IC 443, the Jellyfish Nebula, and the nearby remnant G189.6+3.3 as a likely first binary-star supernova pair: two massive stars that exploded within the same interstellar cloud, about 30–50 light-years apart. IC 443 is estimated at 8,000–9,000 years old, while G189.6+3.3 is older (20,000–110,000 years). The odds of a random alignment are ~1 in 1,000, suggesting a genuine binary progenitor and providing insights into how massive binary stars evolve and end their lives.

Bremont Unveils Hawking-Backed Supernova Limited Edition
business1 month ago

Bremont Unveils Hawking-Backed Supernova Limited Edition

Bremont debuts the Supernova Hawking Limited Edition to celebrate Stephen Hawking, limited to 600 pieces; features a 41mm ultra-black DLC-coated 904L steel case, black ceramic bezel, meteorite sub-dials, and Hawking’s name with his black hole entropy equation on the dial. Powered by the BC77 (Sellita SW500-based) movement at 28,800 bph with a 62-hour power reserve and 100m water resistance. Availability begins July 26, 2026; price US$8,850 on rubber strap and US$9,150 on bracelet; part of Bremont’s Hawking family collaboration.

Neutrinos Carry the Hidden Energy of Core-Collapse Supernovae
astronomy1 month ago

Neutrinos Carry the Hidden Energy of Core-Collapse Supernovae

Core-collapse supernovae emit the vast majority of their energy as neutrinos rather than light—about 99% versus 0.1–1% in photons—because electron capture in the collapsing core produces neutrinos that escape with little interaction. This neutrino burst powers the explosion and confirms the energy budget, as demonstrated by SN 1987A's detections; with detectors like Hyper-Kamiokande and IceCube, a future galactic SN would yield millions of neutrinos, making neutrinos the primary energy carrier in these events.

Astronomers catch a magnetar being born inside a supernova via a rapid brightness chirp
science1 month ago

Astronomers catch a magnetar being born inside a supernova via a rapid brightness chirp

Astronomers observed a distinctive four-peaked, accelerating ‘chirp’ in the light from supernova SN 2024afav, interpreted as the birth of a magnetar—an ultra-mense, highly magnetized neutron star—hidden in the exploding star. The signal fits a model where material falling back formed a tilted accretion disk around the magnetar, whose frame-dragging (Lense–Thirring precession) causes the disk to wobble and periodically modulate the supernova’s brightness. From this, the magnetar is inferred to rotate about 4.2 milliseconds and possess a magnetic field about 300 trillion times stronger than Earth's. While this provides strong evidence for magnetars powering some superluminous supernovae, it may not apply to all such events, and future surveys like the Rubin Observatory will seek more examples to map how often magnetars form in stellar explosions.

Silent Messengers: Neutrinos Illuminate Hidden Galactic Explosions
space1 month ago

Silent Messengers: Neutrinos Illuminate Hidden Galactic Explosions

Avi Loeb explains that neutrinos from Galactic supernovae penetrate interstellar dust and reveal explosions that optical observations often miss. The 1987 SN 1987A produced 24 neutrinos detected by Kamiokande-II, IMB, and Baksan, enabling estimates of the explosion’s energy and the newborn neutron star’s properties. Today’s and forthcoming detectors—Super-Kamiokande, JUNO, IceCube, Hyper-Kamiokande, and DUNE—could observe thousands to tens of thousands of events from a Milky Way supernova, allowing measurements of neutrino masses and oscillations as well as the neutron star’s mass, radius, and binding energy. Webb’s 2022 observations of a neutron-star signature in SN 1987A underscore the potential of neutrino astronomy for probing fundamental physics and stellar remnants.

Feeble Radio Whispers Reveal the Blue Eye Pulsar After Decades of Silence
space1 month ago

Feeble Radio Whispers Reveal the Blue Eye Pulsar After Decades of Silence

Astronomers using the MeerKAT telescope detected faint radio pulses from the central compact object 1E 1207.4-5209—the Blue Eye Pulsar—located about 10,000 light-years away in the Milky Way. The neutron star emits radio waves every 424 milliseconds, matching its rotation and suggesting that some radio-quiet central compact objects can produce detectable radio emission under certain magnetic-field conditions, possibly triggered by a 2015 spin glitch. The finding implies a larger population of ultra-faint pulsars in the galaxy and could help explain missing pulsars in some supernova remnants, with the study published in Nature Astronomy on June 25.

Six Explosions Later, a Star Defies Explanation
astronomy2 months ago

Six Explosions Later, a Star Defies Explanation

A star designated iPTF14hls, first seen in 2014 as a supernova, has since exploded at least six times, with its brightness peaking multiple times over about 1,000 days while staying at a steady 5,000–6,000 K. Archival data reveal a 1954 explosion at the same location, and the star—at least 50 solar masses—appears to eject material far more slowly than typical supernovae. Several ideas (antimatter burning, pulsational pair-instability, magnetar with evolving fields) fail to explain all features. The star faded into a remnant nebula by 2018, and the Hubble Space Telescope continues to monitor the site.