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Gravitational forces of the Sun and Moon deform the Earth’s shape tides in the oceans, atmosphere, and solid earth Tidal effect of the Moon: Earth and Moon are coupled by gravitational attraction: each one rotates around the center of mass of the pair. The rotation of the Earth around that center of mass induces a centrifugal acceleration directed away from the Moon The Moon produces a gravitational attraction on the Earth The resulting force (centrifugal acceleration + gravitational attraction) is responsible for the tides Tidal effect of the Sun: same principle but 45% smaller effect because of larger Earth-Sun distance Tides

Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

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Page 1: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

• Gravitational forces of the Sun andMoon deform the Earth’s shape ⇒tides in the oceans, atmosphere, andsolid earth

• Tidal effect of the Moon:– Earth and Moon are coupled by

gravitational attraction: each onerotates around the center of mass ofthe pair.

– The rotation of the Earth around thatcenter of mass induces a centrifugalacceleration directed away from theMoon

– The Moon produces a gravitationalattraction on the Earth

– The resulting force (centrifugalacceleration + gravitational attraction)is responsible for the tides

• Tidal effect of the Sun: same principlebut 45% smaller effect because oflarger Earth-Sun distance

Tides

Page 2: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Tides• Earth rotation (24 hr) combined

with Moon revolution (~27 days)=> major tidal component is semi-diurnal (M2 = 12 hr 25 min)

• Ocean tides: effect of oceansurface, amplitude of largestcomponent = several meters

• Solid Earth tides: effect on thesolid Earth surface, amplitude,amplitude of largest component~10-50 cm

• By-product of ocean tides: oceantide loading = elastic deformationof the Earth crust due to variationsof ocean water column: up to 15-20 cm near the coast

The ocean tides for harmonic M2 (period of 12 hours and 25 minutes) . The colorrepresent the amplitude and the contour lines indicate the phase lag of the tides with

a spacing of 60 degrees. (Doc. H.G. Scherneck)

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Day of year, 1999

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Water height variations in Brest (France) measured by a tide gauge (October 1999)

Page 3: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Example: ocean tideloading in Brittany, France

Page 4: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Measuring gravity• XVIIth century: pendulum clocks had to be

tuned when moved from Paris (49N) toCayenne (5N) ⇒ first gravity measurementsmade with a pendulum using:

• Absolute measurements: Acceleration of amass in free fall

• Relative measurements:– Extension of a spring (w.r.t. a reference

position)– Levitation of a metal mass in an

electromagnetic field = supraconductinggravimeters

⇒ Need for reference sites where absolute gravityis known

g

lT !2= T = period

l = wire length

relative measurement

absolute measurement

Page 5: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Relative gravity measurements• Mobile masses attached to springs:

– Stable: Measurement of the extensionof the spring (Scintrex)

– Unstable: Measurement of thedisplacement to apply to the spring tobring it back to an equilibriumposition (LaCoste & Romberg)

• Mechanical properties of springsdepend on temperature ⇒ thermostat

• Perfect leveling necessary• Elasticity of springs vary with age ⇒

instrumental drift– Complex, function of age,

transportation, etc.– ~ linear for spring-based gravimeters– Specific to each gravimeter

• Precision ~ 0.01 mGal

LaCoste & Romberg gravimeter

Page 6: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Absolute gravity measurements• Most common technique:

– Glass prism in free fall– Atomic clock => timing of the fall– G = 8H / (DT2 –Dt2)

• Precision ~1 µGal [~ 3 mm]• Transportable, but not easily portable, unlike

relative gravimeters.

Page 7: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s
Page 8: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Precision of ground-basedgravity measurements

Page 9: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Satelliteorbitography

• Orbit of artificial satellites are perturbed by variations of thegravity field.

• Therefore, precise measurements of their trajectory ⇒ gravityfield

• “Geodetic” satellites and ground tracking network ⇒estimation of precise orbit ⇒ restitution of gravity field

• Satellite trajectory derived from Satellite Laser Ranging (SLR) SLR at the Goddard Geophysical and Astronomical Observatory. The twolaser beams are coming from the network standard SLR station, MOBLAS-7

(MOBile LASer) and the smaller TLRS-3 (Transportable Laser RangingSystem) during a collocation exercise.Tracking a satellite with a network of SLR stations

Starlette, a geodetic satelliteLaunched in 1975, 48 cm diameter, 47 kg

Page 10: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

A global gravity field from space…• Current version of global gravity field = GRIM5 [21 satellites, data since 1971, precision

3 mGals]• Advantage = global coverage

Page 11: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Recent space missions

• Obectives are to improve:– Temporal resolution:

atmospheric mass redistribution, oceancirculation, sea level changes and thevisco-elastic response of the Earth'slithosphere to past and present loads

– Spatial resolution from space• Plus atmospheric research• CHAMP• GRACE

Page 12: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

CHAMP• CHAllenging Minisatellite Payload• German (GFZ-Potsdam) small

satellite mission launched in July2000.

• Included instruments:magnetometer, accelerometer, GPSreceiver, laser retro reflector andion drift meter.

• Low altitude, near polar orbit• Continuous GPS satellite-to-

satellite tracking ability• On-board measurements of non-

gravitational orbit perturbations

Page 13: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

GRACE

• Gravity Recovery And ClimateExperiment

• Launched in March 2002 byNASA/DLR.

• Two identical spacecrafts flying about220 km apart in a polar orbit 500 kmabove the Earth.

• Included instruments: K-Band rangingsystem, accelerometer, GPS receiver,laser retro-reflector, star camera, coarseEarth and Sun sensor, ultra stableoscillator, and center of mass trimassembly.

• Gravity field found by highly accuratemeasurements of the distance betweenthe 2 satellites using GPS and amicrowave ranging system

Page 14: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Satellite altimetry and the geoid• Direct measurement of the ocean

surface using satellites• Satellite carries radar ⇒ ocean –

satellite range• Ground tracking system ⇒ ellipsoid –

satellite distance• Difference = ocean – ellipsoid

distance = dynamic topography• Contains:

– Oceanographic effects: waves,currents, tides

– Gravimetric effects = the geoid• Precision:

– SEASAT (1979) = 10 cm– TOPEX-POSEIDON (1992) = 5 cm– JASON (launched in 2002) < 5 cm

• Advantages: precision, coverage

Page 15: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Satellite altimetry

Seafloor topography derived from Seasat altimetric measurements

Page 16: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

Satellite altimetryand the geoid

• Long wavelength → mantle convection• Short wavelength → ocean floor topography• http://topex.ucsd.edu/marine_grav/mar_grav.html

Page 17: Gravitational forces of the Sun and Moon deform the Earth ...web.ics.purdue.edu/~ecalais/teaching/eas450/Gravity3.pdf · •Gravitational forces of the Sun and Moon deform the Earth’s

What have we learned?• The Earth’s gravity is the result of its mass, its rotation,

and its (ellipsoidal) shape.• The Earth’s gravity field is associated with a potential.• The geoid is the particular equipotential surface that best

fits the mean sea level (= the horizontal)• Relationship between geoid and gravity• Gravity and geoid “height” vary:

– As a function of mass distribution (in space and time)– As a function of position (e.g. altitude)

• Direct measurements:– Gravity: up to 1 µGal– Geoid height : up to 5 cm