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THREE-DIMENSIONAL ORTHOGONAL COORDINATE SYSTEM
Oblate spheroidal harmonics; Oblate spheroidal coordinate system
  • Figure 2: Plot of the oblate spheroidal coordinates μ and ν in the ''x''-''z'' plane, where φ is zero and ''a'' equals one. The curves of constant ''μ'' form red ellipses, whereas those of constant ''ν'' form cyan half-hyperbolae in this plane. The ''z''-axis runs vertically and separates the foci; the coordinates ''z'' and ν always have the same sign. The surfaces of constant μ and ν in three dimensions are obtained by rotation about the ''z''-axis, and are the red and blue surfaces, respectively, in Figure 1.
  • Figure 3: Coordinate isosurfaces for a point P (shown as a black sphere) in the alternative oblate spheroidal coordinates (σ, τ, φ). As before, the oblate spheroid corresponding to σ is shown in red, and φ measures the azimuthal angle between the green and yellow half-planes. However, the surface of constant τ is a full one-sheet hyperboloid, shown in blue. This produces a two-fold degeneracy, shown by the two black spheres located at (''x'', ''y'', ±''z'').
  • (1.09, −1.89, 1.66)}}.

oblate      
n. oblato
Mars         
  • Curiosity]]'' rover’s robotic arm showing drill in place, February 2013
  • Mars seen through an 16-inch amateur telescope, at 2020 opposition
  • Ingenuity]]'' helicopter (left) at [[Wright Brothers Field]], 2021
  • Mars without (on left) and with a global dust storm in July 2001 (on right), as seen by the Hubble Space Telescope
  • [[Valles Marineris]], taken by the ''[[Viking 1]]'' probe
  • Edge-on view of Mars atmosphere by ''Viking 1'' probe
  • ♂
  • 600x600px
  • abbr=on}} across.
  • Scoop of Mars soil by ''Curiosity'', October 2012
  • left
  • 300x300px
  • abbr=on}}, comparable in volume to the [[Great Bear Lake]].
  • Orbit of Mars and other Inner Solar System planets
  • invasion of Earth]] by fictional Martians.
FOURTH PLANET IN THE SOLAR SYSTEM FROM THE SUN
Planet Mars; Sol 4; Fourth planet; 4th planet; Sol IV; Physical characteristics of Mars; Mars (Planet); Mars (planet); Oblate Mars; Hydrology of Mars; Mars/Planet; 2003 opposition of Mars; Magnetosphere of Mars; Opposition of Mars; Mars surface features; Mars opposition; Sol-4; Structure of Mars; The planet Mars; Interior of mars; Mars interior; Habitability of Mars
Marte
Benedictine         
  • Montserrat]]
  • [[Abbot Suger]] (c. 1081 – 1135) in a medieval stained-glass window
  • [[Benedict of Aniane]] (747–821).
  • Benedictine nuns make their first profession of vows.
  • [[Bernard of Clairvaux]] (1090–1153) featured in a 13th-century illuminated manuscript
  • [[Saint Boniface]] (c. 680 – 750), [[Pope Gregory I]] (c. 540 – 604, pope 590–604), [[Adalbert of Egmond]] (8th century) and priest Jeroen van Noordwijk, depicted in a 1529 painting by Jan Joostsz van Hillegom currently on display at the [[Frans Hals Museum]]
  • [[Bonifatius Becker]]
  • Self portrait of [[Matthew Paris]] (c. 1200 – 59)
  • The monks of Our Lady of Clear Creek Monastery, in Hulbert Oklahoma.
  • Dom Pérignon]]
  • Friary of San Marco]] [[Florence]].
  • Carolingian manuscript]], c. 840, depicting [[Rabanus Maurus]] (left), supported by [[Alcuin]] (middle), presenting his work to [[Otgar of Mainz]]
  • Late Gothic]] sculpture of [[Rupert of Salzburg]] (c. 660 – 710)
  • The two sides of a ''Saint Benedict Medal''
  • Cardinal Schuster.
ROMAN CATHOLIC RELIGIOUS ORDER
Benedictine monk; Benedictine order; Benedictine monks; Benedictian; Benedictine Order; St. Benedict's monks; Order of St Benedict; Benedictine; Olivetian; Benedictine religious order; O.S.B.; Order of St. Benedict; Benedictine monastery; Black Monks; Black Monk; Benedictine abbey; Order of St. Benedictine; Black monks; Congregation of St. Justina of Padua; Black Benedictines; Oblates of Saint Frances of Rome; Collatines; O. S. B.; Ordo Sancti Benedicti; Benedictine monasticism; Benedictine monasteries; Benedictine nuns; Benedictinian Order; Benedictinians; Benedictinian; Oblates of St. Benedict; Benedictine centuries; Benedictine spirituality; Obl.S.B.; Oblate of Saint Benedict; Oblates of St Benedict; Benedictine nun; O.S.B.Cas.; Black monk; Benedictine Nuns; Order of Saint Benedict
benedictino

تعريف

Prolate
·vt To Utter; to Pronounce.
II. Prolate ·adj Stretched out; extended; especially, elongated in the direction of a line joining the poles; as, a prolate spheroid;
- opposed to oblate.

ويكيبيديا

Oblate spheroidal coordinates

Oblate spheroidal coordinates are a three-dimensional orthogonal coordinate system that results from rotating the two-dimensional elliptic coordinate system about the non-focal axis of the ellipse, i.e., the symmetry axis that separates the foci. Thus, the two foci are transformed into a ring of radius a {\displaystyle a} in the x-y plane. (Rotation about the other axis produces prolate spheroidal coordinates.) Oblate spheroidal coordinates can also be considered as a limiting case of ellipsoidal coordinates in which the two largest semi-axes are equal in length.

Oblate spheroidal coordinates are often useful in solving partial differential equations when the boundary conditions are defined on an oblate spheroid or a hyperboloid of revolution. For example, they played an important role in the calculation of the Perrin friction factors, which contributed to the awarding of the 1926 Nobel Prize in Physics to Jean Baptiste Perrin. These friction factors determine the rotational diffusion of molecules, which affects the feasibility of many techniques such as protein NMR and from which the hydrodynamic volume and shape of molecules can be inferred. Oblate spheroidal coordinates are also useful in problems of electromagnetism (e.g., dielectric constant of charged oblate molecules), acoustics (e.g., scattering of sound through a circular hole), fluid dynamics (e.g., the flow of water through a firehose nozzle) and the diffusion of materials and heat (e.g., cooling of a red-hot coin in a water bath)