Gravity and geodesy form the backbone of geophysics, helping us understand Earth's shape, internal structure, and dynamics. This unit explores fundamental principles like gravitational potential and anomalies, as well as measurement techniques using satellites and ground-based surveys.
From Newton's law of universal gravitation to modern satellite missions, we'll examine how gravity studies have evolved. We'll also dive into practical applications in resource exploration, natural hazard assessment, and monitoring Earth's systems, highlighting the field's importance in geoscience.
Explores the fundamental principles and applications of gravity and geodesy in the context of geophysics
Focuses on understanding the Earth's gravity field, its variations, and how it relates to the planet's shape, internal structure, and dynamics
Covers key concepts such as gravitational potential, gravity anomalies, and geodetic reference systems
Examines the techniques used to measure and model the Earth's gravity field, including satellite-based methods and ground-based surveys
Discusses the implications of gravity and geodesy in various geophysical applications, such as resource exploration, natural hazard assessment, and Earth system monitoring
Key Concepts and Definitions
Gravity: The force of attraction between two masses, governed by Newton's law of universal gravitation
Gravitational potential: The work required to move a unit mass from infinity to a given point in a gravitational field
Geoid: An equipotential surface that closely approximates the mean sea level and represents the shape of the Earth
Gravity anomaly: The difference between the observed gravity at a location and the theoretical gravity predicted by a reference model
Geodesy: The science of accurately measuring and understanding the Earth's geometric shape, orientation in space, and gravity field
Reference ellipsoid: A mathematical model that approximates the shape of the Earth, used as a reference for geodetic calculations
Isostasy: The state of gravitational equilibrium between the Earth's crust and the underlying mantle, assuming a fluid-like behavior over geological timescales
Historical Background
Early observations of the Earth's shape and gravity by ancient Greek scholars, such as Eratosthenes and Aristotle
Newton's formulation of the law of universal gravitation in the 17th century, providing a mathematical foundation for understanding gravity
The development of geodetic techniques in the 18th and 19th centuries, including triangulation and leveling surveys
The establishment of the first international scientific organizations dedicated to geodesy, such as the International Association of Geodesy (IAG) in 1864
The advent of satellite-based methods in the 20th century, revolutionizing the study of Earth's gravity field and shape
Launch of dedicated gravity field missions, such as CHAMP (2000), GRACE (2002), and GOCE (2009)
Improved global gravity field models and insights into Earth's interior structure and dynamics
Earth's Gravity Field
Varies in strength and direction across the Earth's surface due to factors such as latitude, elevation, and mass distribution
Influenced by the Earth's rotation, causing a centrifugal force that opposes gravity and leads to an equatorial bulge
Affected by the uneven distribution of mass within the Earth, including the core, mantle, and crust
Exhibits anomalies due to local variations in density, such as those caused by mountains, ocean trenches, and subsurface geological structures
Continuously evolving due to processes such as glacial isostatic adjustment, sea-level change, and tectonic deformation
Described using spherical harmonic expansions, which decompose the gravity field into a series of wavelengths and amplitudes
Geodetic Measurements and Techniques
Terrestrial techniques:
Gravity measurements using absolute and relative gravimeters
Leveling surveys to determine height differences and establish vertical datums
GNSS (Global Navigation Satellite System) positioning for precise point coordinates
Airborne and shipborne surveys:
Gravity measurements using specialized gravimeters mounted on aircraft or ships
Allows for regional-scale mapping of gravity anomalies and crustal structure
Satellite-based methods:
Satellite altimetry to measure the shape of the ocean surface, which is closely related to the geoid
Satellite gravimetry missions (CHAMP, GRACE, GOCE) to map the global gravity field with unprecedented accuracy and resolution
Satellite laser ranging (SLR) to precisely track the orbits of satellites and infer changes in the Earth's gravity field over time
Applications in Geophysics
Exploration geophysics:
Mapping subsurface density variations to identify potential oil, gas, and mineral resources
Detecting geological structures such as faults, folds, and sedimentary basins
Solid Earth geophysics:
Investigating the structure and composition of the Earth's interior, including the crust, mantle, and core
Studying plate tectonics, earthquakes, and volcanic activity
Hydrological and cryospheric applications:
Monitoring changes in groundwater storage, soil moisture, and snow/ice mass using time-variable gravity measurements (GRACE mission)
Assessing the impacts of climate change on the Earth's water cycle and sea-level rise
Geodynamics:
Understanding the Earth's dynamic processes, such as mantle convection, glacial isostatic adjustment, and tidal deformation
Investigating the coupling between the solid Earth, oceans, and atmosphere
Mathematical Models and Calculations
Newton's law of universal gravitation: F=Gr2m1m2, where F is the gravitational force, G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between their centers
Gravitational potential: V(r)=−rGM, where V(r) is the potential at a distance r from a point mass M, and G is the gravitational constant
Poisson's equation: ∇2V=−4πGρ, relating the gravitational potential V to the density distribution ρ, where ∇2 is the Laplace operator
Spherical harmonic expansion of the gravitational potential: V(r,θ,λ)=rGM∑n=0∞∑m=0n(rR)nPnm(cosθ)(Cnmcosmλ+Snmsinmλ), where R is the reference radius, Pnm are the associated Legendre functions, and Cnm and Snm are the spherical harmonic coefficients
Geodetic reference systems and transformations, such as the International Terrestrial Reference Frame (ITRF) and the Earth Gravitational Model (EGM)
Current Research and Future Directions
Development of next-generation satellite missions for gravity field mapping, such as GRACE-FO (launched in 2018) and future concepts like GRACE-I and MAGIC
Improvement of global gravity field models, incorporating data from multiple satellite missions and ground-based measurements
Integration of gravity data with other geophysical observations (seismic, magnetic, electromagnetic) for a more comprehensive understanding of the Earth's interior
Advancements in computational methods and data processing techniques, enabling higher-resolution and more accurate gravity field solutions
Interdisciplinary research on the interactions between the solid Earth, oceans, atmosphere, and cryosphere, using gravity as a unifying observation
Application of gravity and geodesy to the exploration of other planetary bodies, such as the Moon, Mars, and icy satellites of the outer solar system
Contributions to the United Nations Sustainable Development Goals, particularly in the areas of water resources management, natural hazard mitigation, and climate change adaptation