RESEARCH BASE

Search 3,721 documents across 34 fields — every claim tier-rated by evidence

3,721 Documents 34 Sections 43,625 Citations 34,852 Keywords Indexed 4 Evidence Tiers

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.

20 results for "nitrogen isotopes"

G_4_09 Verified Modern Frameworks

G_4_09 — Bioarchaeology and Forensic Anthropology: Reading the Dead

Bioarchaeology—the study of human remains from archaeological contexts—transforms skeletons from anonymous objects into biographical records of individual lives. Through stable isotope analysis of bone and tooth enamel,

bioarchaeology isotope analysis strontium carbon isotopes nitrogen isotopes oxygen isotopes
G_1_04 Verified Modern Frameworks

G_1_04 — Isotope Analysis and Provenance Studies

Isotope analysis — the measurement of ratios of stable or radiogenic isotopes preserved in human bone, tooth enamel, animal remains, ceramics, metals, and organic residues — has become one of the most powerful tools in m

isotope analysis stable isotopes strontium isotopes oxygen isotopes carbon isotopes nitrogen isotopes
G_1_07 Verified Modern Frameworks

G_1_07 — Stable Isotope Analysis and Ancient Diets

Stable isotope analysis of human and animal remains — primarily the measurement of carbon ($\delta^{13}$C), nitrogen ($\delta^{15}$N), and sulfur ($\delta^{34}$S) isotope ratios in bone collagen, tooth enamel, hair kerat

stable isotopes carbon isotopes nitrogen isotopes sulfur isotopes paleodiet diet reconstruction
ZF_1_16 Verified Oceanography

ZF_1_16 — Paleoceanography and Foraminifera: Reconstructing Ancient Oceans from Microfossil Archives

Paleoceanography — the study of the history of the oceans and their role in Earth's climate system through geological time — relies fundamentally on the geochemical analysis of foraminifera (single-celled protists with c

paleoceanography foraminifera oxygen isotopes δ18O δ13C ocean temperature
ZF_2_07 Verified Oceanography

ZF_2_07 — Marine Microbiology and Plankton

Marine microorganisms — bacteria, archaea, protists, viruses, and microscopic algae — constitute the invisible foundation of ocean life, driving global biogeochemical cycles, producing roughly half of the world's oxygen,

marine microbiology plankton phytoplankton zooplankton cyanobacteria diatom
ZF_4_08 Verified Oceanography

ZF_4_08 — Ocean Acidification Paleoclimate Record

Ocean acidification — the decrease in seawater pH caused by absorption of atmospheric CO₂ — is not only a modern phenomenon but has occurred repeatedly throughout Earth's history, leaving distinctive signals in the geolo

ocean acidification pH paleoclimate PETM Paleocene-Eocene Thermal Maximum carbonate compensation depth
ZF_4_15 Verified Oceanography

ZF_4_15 — Ocean Sediments: Deep-Sea Cores, Proxy Records, and Paleoclimate

Ocean sediments are the Earth's most comprehensive climate archive — a continuous record of planetary conditions extending back over 200 million years, slowly accumulated grain by grain on the deep seafloor at rates of m

ocean sediments deep-sea core marine sediment paleoclimate proxy foraminiferal isotopes oxygen isotopes
ZF_4_14 Verified Oceanography

ZF_4_14 — Harmful Algal Blooms: Red Tides, Toxins, and Eutrophication

Harmful algal blooms (HABs) — rapid proliferations of microscopic algae (phytoplankton) or cyanobacteria that produce toxins, deplete oxygen, or otherwise damage marine ecosystems, fisheries, and human health — are incre

harmful algal bloom HAB red tide algal toxin eutrophication paralytic shellfish poisoning
Q_2_06 Verified Cosmology & Physics

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

nucleosynthesis Big Bang nucleosynthesis stellar nucleosynthesis supernova nucleosynthesis r-process s-process
Q_3_13 Verified Cosmology & Physics

Q_3_13 — Interstellar Objects: 'Oumuamua, Borisov, and Interstellar Visitors

Interstellar objects (ISOs) are bodies — asteroids, comets, or other macroscopic objects — that originate in other star systems and pass through our solar system on unbound, hyperbolic trajectories. While the theoretical

interstellar object 'Oumuamua Borisov 1I 2I ISO
Q_3_17 Verified Cosmology & Physics

Q_3_17 — Titan: Prebiotic Chemistry on Saturn's Largest Moon

Titan, Saturn's largest moon (diameter 5,150 km — larger than Mercury), is the only body in the solar system besides Earth with stable surface liquids and a dense nitrogen-dominated atmosphere. Discovered by Christiaan H

Titan Saturn prebiotic chemistry Cassini-Huygens methane cycle tholin
ZB_3_21 Verified Ecology & Biology

ZB_3_21 — Soil Microbiome

The soil microbiome encompasses the entire community of microorganisms inhabiting soil — bacteria, archaea, fungi, protists, and viruses — constituting the most biodiverse ecosystem on Earth. [KEY FINDING] A single gram

soil microbiome rhizosphere mycorrhiza bacteria fungi archaea
ZB_3_09 Verified Ecology & Biology

ZB_3_09 — Mutualism and Cooperation in Nature

Mutualism — an interspecific interaction in which both partners benefit — is one of the most important ecological relationships on Earth, underpinning ecosystem function from coral reefs to forests to the human gut. The

mutualism symbiosis cooperation reciprocal altruism cleaner fish mycorrhiza
ZB_3_12 Verified Ecology & Biology

ZB_3_12 — Soil Ecology: The Living Skin of the Earth

Soil — far from inert dirt — is the most biologically diverse habitat on Earth, containing an estimated 25–30% of all species on the planet. A single gram of healthy soil harbors approximately 1 billion bacteria (from 10

soil ecology soil microbiome mycorrhizae decomposition soil food web earthworms
G_2_17 Verified Modern Frameworks

G_2_17 — Biogeochemistry and Ancient Environmental Reconstruction

Biogeochemistry — the study of chemical, physical, geological, and biological processes that govern the composition and cycling of elements and compounds in natural environments — provides essential tools for reconstruct

biogeochemistry paleoenvironment proxy isotope sediment core pollen
O_1_14 Verified Earth Anomalies

O_1_14 — Sprites, Elves, and Blue Jets: Upper Atmosphere Transient Luminous Events

Transient Luminous Events (TLEs) are a family of large-scale optical and electrical phenomena occurring in the upper atmosphere (stratosphere, mesosphere, and lower ionosphere, ~20-100 km altitude) above active thunderst

sprites elves blue jets transient luminous events TLE upper atmosphere
R_1_09 Verified Biology & Evolution

R_1_09 — The Great Oxidation Event: Oxygen, Cyanobacteria, and Earth's Atmospheric Transformation

The Great Oxidation Event (GOE), occurring approximately 2.4–2.1 billion years ago during the Paleoproterozoic, was the most dramatic chemical transformation in Earth's history — atmospheric oxygen rose from trace levels

Great Oxidation Event GOE cyanobacteria oxygenic photosynthesis atmospheric oxygen banded iron formations
S_1_21 Verified Future Technology

S_1_21 — Quantum Sensors and Metrology

Quantum sensors exploit the extreme sensitivity of quantum systems — atoms, ions, photons, superconducting circuits, and spin defects — to measure physical quantities (time, frequency, magnetic and electric fields, gravi

quantum sensor quantum metrology atom interferometer optical clock nitrogen-vacancy center SQUID
F_2_06 Verified Lost Connections

F_2_06 — Tin Sources and the Bronze Age Mystery

The Bronze Age (c. 3300–1200 BCE) depended fundamentally on tin — the scarce metal alloyed with copper to produce bronze (typically 88–92% copper, 8–12% tin). While copper was widely available across the Mediterranean, N

tin cassiterite Bronze Age bronze copper-tin alloy Cornwall
ZA_4_19 Verified Physics & Quantum

ZA_4_19 — Cryogenics and Low-Temperature Physics

Cryogenics — the production and behavior of materials at temperatures below ~120 K (−153 °C) — began with Heike Kamerlingh Onnes (Leiden), who first liquefied helium on July 10, 1908, reaching 4.2 K and opening the ultra

cryogenics low temperature liquid helium liquid nitrogen Kamerlingh Onnes absolute zero