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Search 3,721 documents across 34 fields — every claim tier-rated by evidence
3,633 are the core, quality-scored corpus (34 lettered sections — see How We Work); the remaining 88 are cross-corpus synthesis documents (68 InterDocs, 12 Connections, 8 Theories) also indexed here.
31 results for "Vela supernova" — page 1 of 2
E_1_14 — Supernovae in Human History: Crab Nebula, SN 1006, Vela
Supernovae — the catastrophic explosions of massive stars (core-collapse, Type II/Ib/Ic) or white dwarfs exceeding the Chandrasekhar mass limit (thermonuclear, Type Ia) — are among the most energetic events in the univer
E_1_08 — Ancient Supernovae and Their Cultural Impact
Supernovae — the explosive deaths of massive stars — are among the most energetic events in the universe, capable of briefly outshining entire galaxies. When they occur within our galaxy at distances of a few thousand li
ZH_4_17 — Supernova Records Cross-Validation: Historical Observations and Modern Remnant Identification
Historical supernova observations — "guest stars" (kè xīng, 客星) recorded in Chinese, Japanese, Korean, Arabic, and European sources — provide a unique dataset for cross-validating astrophysical models of supernova remnan
ZH_2_01 — Chinese Astronomical Records: Supernovae, Comets, Guest Stars
China produced the longest continuous tradition of systematic astronomical observation in human history — spanning from the Shang dynasty oracle bone inscriptions (c. 1200 BCE) through the imperial astronomical bureaus o
Q_2_14 — Gamma-Ray Bursts
Gamma-ray bursts (GRBs) are the most energetic electromagnetic events in the universe — brief, intense flashes of gamma radiation that, when corrected for beaming, release ~10⁴⁴–10⁴⁷ joules in seconds to minutes. First d
Q_2_16 — White Dwarfs, Type Ia Supernovae, and Standard Candles
White dwarfs — the remnant cores of low- and intermediate-mass stars (initial mass < ~8 M☉, ~97% of all stars) — are dense objects supported against gravitational collapse by electron degeneracy pressure, with typical ma
Q_4_16 — Chandrasekhar Limit: White Dwarf Physics and Stellar Death
The Chandrasekhar limit — approximately 1.4 solar masses ($1.4 \, M_\odot$) — is the maximum mass of a stable white dwarf star, the dense remnant left after a low- or intermediate-mass star (initial mass up to ~8 $M_\odo
B_3_14 — Four Horsemen and Apocalyptic Entities: End-Time Beings
Apocalyptic entities — supernatural beings associated with the end of the world, the Last Judgment, and the cosmic battle between good and evil — populate the eschatological traditions of virtually every major religion.
ZH_4_09 — Astronomical Petroglyphs and Rock Art
Humans have carved, painted, and pecked celestial imagery into rock surfaces for at least 10,000 years — and possibly far longer. Astronomical petroglyphs and pictographs are found on every inhabited continent: images of
ZH_2_05 — Japanese and Korean Astronomical Traditions
The astronomical traditions of Japan and Korea developed in close dialogue with Chinese astronomy — but were far from mere copies. Both civilizations adapted Chinese astronomical models, instruments, and calendrical meth
C_1_13 — Sacred Mountains and the Cosmic Mountain
The sacred mountain is one of humanity's most enduring religious symbols — a vertical axis connecting earth and heaven that appears in virtually every major civilization. From Mount Meru at the center of Hindu-Buddhist-J
C_2_08 — Venus / Morning Star Traditions
Venus, the brightest object in the sky after the Sun and Moon, plays a central role in myths across every major civilization. The Sumerians identified Inanna as the planet Venus, whose descent to and return from the unde
ZG_2_05 — Sacred Languages — Sanskrit, Hebrew, Arabic, Latin
Across civilizations, certain languages have been elevated above the ordinary functions of communication to the status of sacred or liturgical languages — vehicles believed to possess special power by virtue of their con
Q_1_15 — Dark Energy Models and Quintessence
The accelerating expansion of the universe, discovered in 1998 via Type Ia supernovae, demands an explanation. The simplest model — Einstein's cosmological constant Λ with equation of state $w = p/\rho = -1$ exactly — fi
Q_1_11 — Cosmological Redshift and the Hubble Law
The discovery that distant galaxies' light is systematically shifted toward longer (redder) wavelengths was the first observational evidence that the universe is expanding. Vesto Slipher's spectroscopic measurements (191
Q_2_13 — Interstellar Medium, Dust, and Nebulae
The space between stars is far from empty — the interstellar medium (ISM) is a complex, dynamic ecosystem of gas, dust, magnetic fields, and cosmic rays that pervades galaxies and plays a central role in stellar birth, d
Q_2_06 — Nucleosynthesis: How the Elements Were Forged
Every element in the periodic table has a specific cosmic origin story. Big Bang nucleosynthesis (BBN) produced hydrogen, helium, and traces of lithium in the first 20 minutes after the Big Bang. Stellar nucleosynthesis
Q_2_07 — Cosmic Distance Ladder: Measuring the Universe
The cosmic distance ladder is a succession of techniques by which astronomers measure distances from nearby stars to the edge of the observable universe — each rung calibrates the next. Trigonometric parallax (reliable t
Q_2_09 — Binary Star Systems and X-Ray Sources
Most stars in the Milky Way exist in binary or multiple-star systems — estimates range from ~50% for solar-type stars to >70% for massive O/B stars. Binary star interactions drive some of the most energetic phenomena in
Q_2_03 — Cosmic Rays and High-Energy Astrophysics
Cosmic rays — high-energy particles from space, mostly protons and atomic nuclei — were discovered by Victor Hess in 1912 via balloon flights that measured ionization increasing with altitude, earning him the Nobel Prize
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