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Gravity of Mars

The gravity of Mars is a natural phenomenon, due to the law of gravity, or gravitation, by which all things with mass around the planet Mars are brought towards it. It is weaker than Earth's gravity due to the planet's smaller mass. The average gravitational acceleration on Mars is 3.721 m/s2, with a global variation range of ~0.059 m/s2.

Measurement
To understand the gravity of Mars, its gravitational field strength g and gravitational potential U are often measured. Simply, if Mars is assumed to be a static perfectly spherical body of radius RM, provided that there is only one satellite revolving around Mars in a circular orbit and such gravitation interaction is the only force acting in the system, the equation would be :\frac{GMm}{r^2}=mr\omega^2, where G is the universal constant of gravitation (commonly taken as G = 6.674 × 10−11 m3 kg−1 s−2), M is the mass of Mars (most updated value: 6.41693 × 1023 kg), m is the mass of the satellite, r is the distance between Mars and the satellite, and \omega is the angular velocity of the satellite, which is also equivalent to \frac{2\pi}{T} (T is the orbiting period of the satellite). Therefore, g = \frac{GM}{R_M^2}=\frac{r^3\omega^2}{R_M^2}=\frac{4r^3\pi^2}{T^2R_M^2}, where RM is the radius of Mars. With proper measurement, r, T, and RM are obtainable parameters from Earth. However, as Mars is a generic, non-spherical planetary body and influenced by complex geological processes, more accurately, the gravitational potential is described with spherical harmonic functions, following convention in geodesy; see Geopotential model. :U(r, \lambda,\psi)= -\frac{GM}{r} \left(1+ \sum_{\ell=2}^{\ell=L} \left ( \frac{R}{r} \right )^\ell \left( C_{\ell 0} P_\ell^0(\sin\psi) + \sum_{m=1}^{+\ell} (C_{\ell m}\cos m\lambda+S_{\ell m}\sin m\lambda)P_\ell^m(\sin \psi) \right) \right), where r,\psi,\lambda are spherical coordinates of the test point. GM could be obtained through observations of the motions of the natural satellites of Mars (Phobos and Deimos) and spacecraft flybys of Mars (Mariner 4 and Mariner 6). which allow calculation of the ratio of solar mass to the mass of Mars, moment of inertia and coefficient of the gravitational potential of Mars, and give initial estimates of the gravity field of Mars. One-way tracking means the data is transmitted in one way to the DSN from the spacecraft, while two-way and three-way involve transmitting signals from Earth to the spacecraft (uplink), and thereafter transponded coherently back to the Earth (downlink). While for the range tracking, it is done through measurement of round trip propagation time of the signal. Combination of Doppler shift and range observation promotes higher tracking accuracy of the spacecraft. The tracking data would then be converted to develop global gravity models using the spherical harmonic equation displayed above. However, further elimination of the effects due to affect of solid tide, various relativistic effects due to the Sun, Jupiter and Saturn, non-conservative forces (e.g. angular momentum desaturations (AMD), atmospheric drag and solar radiation pressure) have to be done, otherwise, considerable errors result. == History ==
History
The latest gravity model for Mars is the Goddard Mars Model 3 (GMM-3), produced in 2016, with spherical harmonics solution up to degree and order 120. Further combination of the two data sets, along with correlation of anomalies with volcanic features (positive anomaly) and deep-printed depression (negative anomaly) assisted by image data allows a degree and order of 18 spherical harmonic solution produced. Further use of spatial a priori constraint method, which had taken the topography into account in solving the Kaula power law constraint, had favored model of up to degree 50 spherical harmonic solution in global resolution (Goddard Mars Model-1, or GMM-1) then the subsequent models with higher completeness and degree and order up to 120 for the latest GMM-3. These factors could lead to offset of the true gravity field. Accurate modeling is thus required to eliminate the offset. Such work is still ongoing. == Static gravity field ==
Static gravity field
Many researchers have outlined the correlation between short-wavelength (locally varying) free-air gravity anomalies and topography. For regions with higher correlation, free-air gravity anomalies could be expanded to higher degree strength through geophysical interpretation of surface features, Free-air gravity anomalies are relatively easier to measure than the Bouguer anomalies as long as topography data is available because it does not need to eliminate the gravitational effect due to the effect of mass surplus or deficit of the terrain after the gravity is reduced to sea level. However, to interpret the crustal structure, further elimination of such gravitational effect is necessary so that the reduced gravity would only be the result of the core, mantle and crust below datum. High correlation is expected for degree over 50 (short-wavelength anomaly) on Mars. Alba Patera, also a volcanic rise, north of the Tharsis Montes, however, produces negative Bouguer anomaly, though its extension is similar to that of Olympus Mons. It has been suggested that the extruded lava could range from andesite (low density) to basaltic (high density) and the composition could change during the construction of the volcanic shield, which contributes to the anomaly. Such setting has already been observed over the famous Syrtis major, which has been inferred to have an extinct magma chamber with 3300 kg m3 underlying the volcano, evident from positive Bouguer anomaly. which cannot be attributed to local isostasy, but rather finite strength of the mantle and density differences in the convection current. which has been evolving with time. The correlation between certain topography anomalies and long-wavelength gravity anomalies, for example, the Mid-Atlantic Ridge and Carlsberg Ridge, which are topography high and gravity high on the ocean floor, thus became the argument for the convection current idea on Earth in the 1970s, though such correlations are weak in the global picture. Another possible explanation for the global scale anomalies is the finite strength of the mantle (in contrast to zero stress), which makes the gravity deviated from hydrostatic equilibrium. For this theory, because of the finite strength, flow may not exist for most of the region that are understressed. And the variations of density of the deep mantle could be the result of chemical inhomogeneities associated with continent separations, and scars left on Earth after the torn away of the Moon. These are the cases suggested to work when slow flow is allowed to happen under certain circumstances. However, it has been argued that the theory may not be physically feasible. == Time-variable gravity field ==
Time-variable gravity field
-condensation cycle of carbon dioxide on Mars between the atmosphere and cryosphere (polar ice cap) operates seasonally. The measured gravitational potential of Mars from orbiters could be generalized as the equation below, : V(\text{Mars})=V(\text{solid planet})+V(\text{seasonal caps}+\text{atmosphere}) where l is the degree while m is the order. More commonly, they are represented in form of Clm in research papers. If we regard the two poles as two distinct point masses, then, their masses are defined as, : M_{NP}=\frac{C_{20}+C_{30}}{2}\,M_\text{Mars} : M_{SP}=\frac{C_{20}-C_{30}}{2}\,M_\text{Mars} Data has indicated that the maximum mass variation of the southern polar cap is approximately 8.4 × 1015 kg, occurring near the autumnal equinox, while for that of the northern polar is approximately 6.2 × 1015 kg, occurring in between the winter solstice and spring equinox. In long term speaking, it has been found that the mass of ice stored in North Pole would increase by (1.4 ± 0.5) × 1011 kg, while in South Pole it would decrease by (0.8 ± 0.6) × 1011 kg. In addition, the atmosphere would have decrease in term of the mass of carbon dioxide by (0.6 ± 0.6) × 1011 kg in long term as well. Due to existence of uncertainties, it is unclear whether migration of material from the South Pole to the North Pole is ongoing, though such a possibility cannot be ruled out. == Tide ==
Tide
The two major tidal forces acting on Mars are the solar tide and Phobos tide. Love number k2 is an important proportional dimensionless constant relating the tidal field acting to the body with the multipolar moment resulting from the mass distribution of the body. Usually k2 can tell quadrupolar deformation. Finding k2 is helpful in understanding the interior structure on Mars. The most updated k2 obtained by Genova's team is 0.1697 ± 0.0009. As if k2 is smaller than 0.10 a solid core would be indicated, this tells that at least the outer core is liquid on Mars, and the predicted core radius is 1520–1840 km. However, current radio tracking data from MGS, ODY and MRO does not allow the effect of phase lag on the tides to be detected because it is too weak and needs more precise measurement on the perturbation of spacecraft in the future. == Geophysical implications ==
Geophysical implications
Crustal thickness , free-air gravity anomaly and crustal density map – Red: gravity high; Blue: gravity low |300x300px No direct measurement of crustal thickness on Mars is currently available. Geochemical implications from SNC meteorites and orthopyroxenite meteorite ALH84001 suggested that mean crustal thickness of Mars is 100–250 km. Viscous relaxation analysis suggested that the maximum thickness is 50–100 km. Such thickness is critical in maintaining hemispheric crustal variations and preventing channel flow. Combination studies on geophysics and geochemistry suggested that average crustal thickness could be down to 50 ± 12 km. Measurement of gravity field by different orbiters allows higher-resolution global Bouguer potential model to be produced. Many are even found to have negative free air gravity anomaly, though evidence has shown that all of them should have experienced gravity high (positive free air gravity anomaly). which represents a global average value. Lateral variation of the crustal density should exist. For example, over the volcanic complexes, local density is expected to be as high as 3231 ± 95 kg m−3, which matched the meteorite data and previous estimations. In addition, the density of the northern hemisphere is in general higher than that of the southern hemisphere, which may imply that the latter is more porous than the former. To achieve the bulk value, porosity could play an important role. If the mineral grain density is chosen to be 3100 kg m−3, 10% to 23% porosity could give a 200 kg m−3 drop in the bulk density. If the pore spaces are filled with water or ice, bulk density decrease is also expected. A further drop in bulk density could be explained by increasing density with depth, with the surface layer more porous than the deeper Mars, and the increase of density with depth also has geographical variation. == Engineering and scientific applications ==
Engineering and scientific applications
Areoid The areoid is a planetary geoid that represents the gravitational and rotational equipotential figure of Mars, analogous to the concept of geoid ("sea level") on Earth. This has been set as the reference frame for developing the MOLA Mission Experiment Gridded Data Records (MEGDRs), Combination of these two works allows the areoid as well as the MEGDRs to be constructed. Based on the above, the areoid has taken the radius as the mean radius of the planet at the equator as 3396 km. The first man-made object landing on Mars, the Mars 2 lander, crashed for an unknown reason. Since the surface environment of Mars is complex, composed of laterally varying morphological patterns, in order to avoid rock hazard the landing progress should be further assisted by employment of LIDAR on site in determining the exact landing position and other protective measures. ==See also==
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