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Special case of the two-body problem
In classical mechanics, the Kepler problem is a special case of the two-body problem, in which the two bodies interact by a central force that varies in
Kepler_problem
Math theorem about sphere packing
The Kepler conjecture, named after the 17th-century mathematician and astronomer Johannes Kepler, is a mathematical theorem about sphere packing in three-dimensional
Kepler_conjecture
Problem in physics and astronomy
three-body problem is known by a variety of names, such as the problem of two fixed centers, the Euler–Jacobi problem, and the two-center Kepler problem. The
Euler's_three-body_problem
Motion problem in classical mechanics
most prominent example of the classical two-body problem is the gravitational case (see also Kepler problem), arising in astronomy for predicting the orbits
Two-body_problem
Equation giving the form of a central force
the total energy ( E = T + V {\displaystyle E=T+V} ). The traditional Kepler problem of calculating the orbit of an inverse square law may be read off from
Binet_equation
described by the field equations of general relativity. Solving the Kepler problem is essential to calculate the bending of light by gravity and the motion
Two-body problem in general relativity
Two-body_problem_in_general_relativity
Vector used in astronomy
distance between them; such problems are called Kepler problems. Thus the hydrogen atom is a Kepler problem, since it comprises two charged particles interacting
Laplace–Runge–Lenz_vector
German astronomer and mathematician (1571–1630)
Johannes Kepler (27 December 1571 – 15 November 1630) was a German polymath who was an astronomer, mathematician, astrologer, natural philosopher and music
Johannes_Kepler
Celestial orbit whose trajectory is a conic section in the orbital plane
said to be a solution of a special case of the two-body problem, known as the Kepler problem. As a theory in classical mechanics, it also does not take
Kepler_orbit
Orbital mechanics term
mechanics, Kepler's equation relates various geometric properties of the orbit of a body subject to a central force. It was derived by Johannes Kepler in 1609
Kepler's_equation
Class of problems in classical mechanics
repulsive one. This special case of the classical central-force problem is called the Kepler problem. For an inverse-square force, the Binet equation derived
Classical central-force problem
Classical_central-force_problem
Laws describing planetary orbits
astronomy, Kepler's laws of planetary motion give good approximations for the orbits of planets around the Sun. They were published by Johannes Kepler from
Kepler's laws of planetary motion
Kepler's_laws_of_planetary_motion
Hypothetical quantum cosmological effect
in which the trans-Planckian problem is addressed.[citation needed] The key point is that similar trans-Planckian problems occur when the modes occupied
Hawking_radiation
Problem in physics and celestial mechanics
is used if possible. The two-body problem in general relativity is analytically solvable only for the Kepler problem, in which one mass is assumed to be
N-body_problem
Hypothetical topological feature of spacetime
between the two sheets a "bridge". — A. Einstein, N. Rosen, "The Particle Problem in the General Theory of Relativity" For the combined field, gravity and
Wormhole
Laws in physics about force and motion
an inverse-square force law will produce is known as the Kepler problem. The Kepler problem can be solved in multiple ways, including by demonstrating
Newton's_laws_of_motion
Exact solution to the Einstein field equations
accepted as correct. This led Oppenheimer to consider the natural next problem of determining what would happen if a neutron star were so heavy it would
Oppenheimer–Snyder_model
Attraction of masses and energy
suggestion, Newton tackled the problem and was able to prove that ellipses also proved the inverse square relation from Kepler's observations. In 1684, Isaac
Gravity
Field-equations in general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Einstein_field_equations
Hypothetical object of spacetime
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
White_hole
Differentiable manifold with nondegenerate metric tensor
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Pseudo-Riemannian_manifold
Black holes are characterized only by mass, charge, and spin
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
No-hair_theorem
Two interrelated physics theories by Albert Einstein
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Theory_of_relativity
English polymath (1642–1727)
Brackenridge, John Bruce (1996). The Key to Newton's Dynamics: The Kepler Problem and the Principia. University of California Press. p. 74. ISBN 978-0-520-91685-2
Isaac_Newton
General-relativistic effect
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Gravitational_time_dilation
Region in spacetime from which nothing can escape
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Event_horizon
Compact astronomical body
Hubble Space Telescope. Unsolved problem in physics Is physical information lost in black holes? More unsolved problems in physics According to the no-hair
Black_hole
Measured time difference as explained by relativity theory
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Time_dilation
Thought experiment in special relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Twin_paradox
Concept in general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Einstein–Hilbert_action
NASA space telescope for exoplanetology (2009–2018)
zone: Kepler-560b, Kepler-705b, Kepler-1229b, Kepler-1410b, Kepler-1455b, Kepler-1544 b, Kepler-1593b, Kepler-1606b, and Kepler-1638b. The Kepler team
Kepler_space_telescope
Paths of particles in the Schwarzschild solution to Einstein's field equations
Physics portal Classical central-force problem Frame fields in general relativity Kepler problem Two-body problem in general relativity This substitution
Schwarzschild_geodesics
Condition in which spacetime itself breaks down
(returning to one's own past) around the Kerr singularity, which leads to problems with causality like the grandfather paradox. However, processes inside
Gravitational_singularity
Statement of spherically symmetric spacetimes
ISBN 978-94-007-5409-6. Padmanabhan, Thanu (1996). Cosmology and Astrophysics through problems. Cambridge University Press. pp. 8, 150. ISBN 0-521-46783-7. Padmanabhan
Birkhoff's theorem (relativity)
Birkhoff's_theorem_(relativity)
Change in wavelength of light
technique was first described by: Baum, W. A. (1962). McVittie, G. C. (ed.). Problems of extra-galactic research. IAU Symposium No. 15. p. 390. Bolzonella, M
Redshift
Physical constant equal to the speed of light
gravitational interaction in general relativity does not lead to the sorts of problems with the aberration of gravity that Newton was originally concerned with
Speed_of_gravity
Equations in physical cosmology
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Friedmann_equations
Idea that small causes can have large effects
quantum physics, including atoms in strong fields and the anisotropic Kepler problem. Some authors have argued that extreme (exponential) dependence on initial
Butterfly_effect
Theorem in general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Lovelock's_theorem
Theory of gravitation as curved spacetime
Linde 2006 More precisely, these are the flatness problem, the horizon problem, and the monopole problem; a pedagogical introduction can be found in Narlikar
General_relativity
Solution of Einstein field equations
geodesics of the underlying Minkowski space proved very difficult. The problem was given to George Debney to try to solve but was given up by March 1964
Kerr–Newman_metric
Precession of a gyroscope due to a nearby celestial body's rotation affecting spacetime
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Lense–Thirring_precession
Tensor that describes the 4D geometry of spacetime
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Metric tensor (general relativity)
Metric_tensor_(general_relativity)
Key results in general relativity on gravitational singularities
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Penrose–Hawking singularity theorems
Penrose–Hawking_singularity_theorems
Solution of Einstein field equations
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Gödel_metric
Generalization of straight line to a curved space time
possibility of a logically more satisfactory treatment of the combined problem: The problem of the field and that of the motion coincide. Both physicists and
Geodesics in general relativity
Geodesics_in_general_relativity
Tensor used in general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Einstein_tensor
Solution to the Einstein field equations
those radii larger than the radius R of the gravitating body, there is no problem as long as R > rs. For ordinary stars and planets this is always the case
Schwarzschild_metric
Time delay caused by space-time distortion near massive objects
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Shapiro_time_delay
Time scale
Introduction to the mathematics of general relativity S A Klioner (1992), "The problem of clock synchronization - A relativistic approach", Celestial Mechanics
Coordinate_time
Experiments proving existence of atomic nuclei
theory was developed under the name of the Kepler problem. The well-known solutions to the Kepler problem are called orbits and unbound orbits are hyperbolas
Rutherford scattering experiments
Rutherford_scattering_experiments
Formalism in general relativity
simplicial approximation to a vacuum solution. This can be applied to difficult problems in numerical relativity such as simulating the collision of two black holes
Regge_calculus
Tensor describing energy momentum density in spacetime
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Stress–energy_tensor
Coordinate system
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Lemaître_coordinates
^{-1/2}\right]\mathbf {M} ^{-1/2}\mathbf {C} } The method can solve the inverse Kepler problem of determining the force law that corresponds to the orbits that are
Udwadia–Kalaba_formulation
In astrodynamics and celestial mechanics a radial trajectory is a Kepler orbit with zero angular momentum. Two objects in a radial trajectory move directly
Radial_trajectory
Exact gravitational-wave solution to Einstein's field equations
predicted the existence of gravitational waves in 1916. He returned to the problem 20 years later, working with his assistant, Rosen. Einstein and Rosen thought
Einstein–Rosen_metric
Conservation law
only algebraic ones. Similarly to the Laplace–Runge–Lenz vector in the Kepler problem, the Fradkin tensor arises from a hidden symmetry of the harmonic oscillator
Fradkin_tensor
Plane curve: conic section
two given points. The path followed by any particle in the classical Kepler problem is a conic section. In particular, if the total energy E of the particle
Hyperbola
Path of an object through spacetime
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
World_line
Method of solution for certain mechanical problems
additional general conserved quantities; for example, the frequencies of the Kepler problem are degenerate, corresponding to the conservation of the Laplace–Runge–Lenz
Action-angle_coordinates
Physical effect in general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Gravitational_redshift
Effect of general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Frame-dragging
formulation is a method used to solve the two-body Kepler problem. It is a generalized form of Kepler's Equation, extending it to apply not only to elliptic
Universal variable formulation
Universal_variable_formulation
Equation explaining structure of a spherical body of isotropic material
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Tolman–Oppenheimer–Volkoff equation
Tolman–Oppenheimer–Volkoff_equation
Numerical integration scheme for Hamiltonian systems
long-term evolution of chaotic Hamiltonian systems ranging from the Kepler problem to the classical and semi-classical simulations in molecular dynamics
Symplectic_integrator
Keplerian elements Kepler orbit Kepler problem Kepler problem in general relativity Kepler space telescope Kepler Launch Site Kepler photometer Keplerian
List of things named after Johannes Kepler
List_of_things_named_after_Johannes_Kepler
Branch of astrophysics
statistical mechanics. In essence, the fundamental problem of stellar dynamics is the N-body problem, where the N members refer to the members of a given
Stellar_dynamics
Solution to Einstein field equations
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Gravitational_plane_wave
1984 graduate textbook by Robert M. Wald
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
General_Relativity_(book)
Class of exact solutions to Einstein's field equations
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Dust_solution
General relativity equation
Plyatsko (2011). "Can Mathisson-Papapetrou equations give clue to some problems in astrophysics?". arXiv:1110.2386 [gr-qc]. M. Leclerc (2005). "Mathisson-Papapetrou
Mathisson–Papapetrou–Dixon equations
Mathisson–Papapetrou–Dixon_equations
Key result in general relativity
formulations have been rigorously proven, and it is currently an open problem whether the above formulation holds for initial data sets of arbitrary
Positive_energy_theorem
Undergraduate textbook on mathematics and mathematical physics
geometry to solve the Kepler problem. It was written by Stephanie Singer, and published by Birkhäuser in 2001. The Kepler problem in classical mechanics
Symmetry_in_Mechanics
Hypothesis that inertial and gravitational masses are equivalent
Mach's principle Tests of general relativity Unsolved problems in astronomy Unsolved problems in physics Einstein, Albert (2003). The Meaning of Relativity
Equivalence_principle
Physical law
Distance decay Fermi paradox Flux Gauss's law Inverse proportionality Kepler problem Kepler's laws of planetary motion Multiplicative inverse Principle of similitude
Inverse-square_law
Light bending by mass between source and observer
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Gravitational_lens
JSTOR 531520. See J. Bruce Brackenridge, "The key to Newton's dynamics: the Kepler problem and the Principia", (University of California Press, 1995), especially
Hooke–Newton inverse square law controversy
Hooke–Newton_inverse_square_law_controversy
Physics problem related to laws of motion and gravity
Tycho Brahe and Johannes Kepler, Newton introduced later generations to the beginning of the gravitational three-body problem. In Proposition 66 of Book
Three-body_problem
then-poorly-understood theory of general relativity rather than to seriously analyze the problem: Eddington did not believe black holes existed. In 1939, Einstein himself
History_of_black_hole_physics
Physical interaction of charged particles
square, matching a detailed theory developed under the name of the Kepler problem. JJ Thomson had applied some of the ideas in his 1910 paper on beta
Coulomb_scattering
Exact solution for the Einstein field equations
general static spherically symmetric perfect fluid solutions. However, the problem of finding a rotating perfect-fluid interior which can be matched to a
Kerr_metric
Cosmological model
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Milne_model
Hamiltonian formulation of general relativity
ADM formulation. The most common approaches start with an initial value problem based on the ADM formalism. In Hamiltonian formulations, the basic point
ADM_formalism
Linear perturbations to solutions of nonlinear Einstein field equations
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Linearized_gravity
On lattices and sphere packing in Euclidean space
of the Kepler conjecture. It shows that the most space-efficient way to pack spheres is in a pyramid shape. Milnor, J. (1976), "Hilbert's problem 18", in
Hilbert's_eighteenth_problem
Tensor field in Riemannian geometry
Vernon D (1978). "Tensor spherical harmonics on S 2 and S 3 as eigenvalue problems" (PDF). Journal of Mathematical Physics. 19 (12): 2441–2446. Bibcode:1978JMP
Riemann_curvature_tensor
Approximate solution to Einstein's field equations
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Hartle–Thorne_metric
Topics referred to by the same term
types of central-force problems, depending on the physical theory being applied. Classical central-force problem Kepler problem, a special case (inverse-square
Central-force_problem
Classification used in differential geometry and general relativity
{\frac {1}{2}}\,{C^{ab}}_{mn}X^{mn}} Then, it is natural to consider the problem of finding eigenvalues λ {\displaystyle \lambda } and eigenvectors (which
Petrov_classification
Solution of Einstein field equations
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Kasner_metric
Origins of Einstein's gravitation theory
his gravitational theory. For a while, Einstein thought that there were problems with the approach, but he later returned to it and, by late 1915, had published
History_of_general_relativity
Aspect of relativity in physics
Lightman, A.P.; Press, W.H.; Price, R.H.; Teukolsky, S.A. (1975). "Problem 12.16". Problem book in Relativity and Gravitation. Princeton University Press
Gravitational_wave
Force directed to the center of rotation
Brackenridge, John Bruce (1996). The Key to Newton's Dynamics: The Kepler Problem and the Principia. University of California Press. p. 74. ISBN 978-0-520-91685-2
Centripetal_force
Motion extremely close to the speed of light
massless particles such as the photon from those of massive particles (cf. Kepler problem in general relativity). [citation needed] Below are few ultrarelativistic
Ultrarelativistic_limit
Type of horizon in spacetime
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Absolute_horizon
Exact solution in general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Reissner–Nordström_metric
Formalism of general relativity
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
BSSN_formalism
Situation or occurrence located at a specific point in space and time
Special relativity World line Pseudo-Riemannian manifold Phenomena Kepler problem Gravitational lensing Gravitational redshift Gravitational time dilation
Event_(relativity)
Turkish-American theoretical physicist (1926–1994)
ISBN 0306402777, Plenum Publishing Corporation. Group Theory in Non-Linear Problems, NATO Advanced Study Institute, Barut, Asim O. (ed.), 1974, ISBN 9027704120
Asım_Orhan_Barut
KEPLER PROBLEM
KEPLER PROBLEM
Boy/Male
Gaelic
Little champion.
Surname or Lastname
Americanized form of German Möller (see Moeller).German
Americanized form of German Möller (see Moeller).German : habitational name for someone from Melle.German, Jewish (Ashkenazic), and Polish : occupational name for a miller or flour merchant, from an agent derivative of German Mehl ‘flour’.English : variant of Miller.
Surname or Lastname
English
English : variant spelling of Saylor.German : variant spelling of Seiler.
Surname or Lastname
Jewish (eastern Ashkenazic)
Jewish (eastern Ashkenazic) : occupational name from Yiddish tesler ‘carpenter’.English : variant of Tessler.German : variant of Tescher.
Surname or Lastname
English
English : occupational name from Old French telier ‘weaver’, ‘linen-weaver’.German : variant of Tell 2 and 3.Dutch : occupational name for a teller, a marketplace official.Jewish (Ashkenazic) : either a metonymic occupational name for a dish maker or a nickname, from German Teller, Yiddish teler ‘plate’.Catalan : from a derivative of Tell 4.This name is recorded in Beverwijck in New Netherland (Albany, NY) in the mid 17th century.
Surname or Lastname
English
English : variant of Kilner.German, Dutch, and Jewish (Ashkenazic) : variant spelling of Kellner, in any of its senses: ‘cellarman’, ‘steward’, ‘overseer’, or ‘waiter’. In this spelling it is also found as a Czech name.Jewish (Ashkenazic) : occupational name from modern German Kellner or Yiddish kelner ‘waiter’.
Surname or Lastname
English
English : probably a variant of Mellor. Compare Mealor, Mealer.
Surname or Lastname
English
English : probably a variant of Mellor. Compare Mealor, Meeler.
Surname or Lastname
English (Norfolk)
English (Norfolk) : habitational name from Madehurst in Sussex, which gets its name from Old English mǣd ‘meadow’ (see Mead 1) + hyrst ‘wooded hill’. This place name appears in 12th-century records in the Normanized form Medl(i)ers. The surname is found in Norfolk as early as the 13th century in the form de Medlers; the landowning family that bore it was in vassalage to the Earl of Surrey, who had large estates in both Sussex and Norfolk.
Surname or Lastname
German
German : nickname from the small medieval coin known as the häller or heller because it was first minted (in 1208) at the Swabian town of (Schwäbisch) Hall. Compare Hall.Jewish (Ashkenazic) : habitational name for someone from Schwäbisch Hall.German : topographic name for someone living by a field named as ‘hell’ (see Helle 3).English : topographic name for someone living on a hill, from southeastern Middle English hell + the habitational suffix -er.Dutch : from a Germanic personal name composed of the elements hild ‘strife’ + hari, heri ‘army’.Jewish (Ashkenazic) : nickname for a person with fair hair or a light complexion, from an inflected form, used before a male personal name, of German hell ‘light’, ‘bright’, Yiddish hel.
Female
English
Irish surname transferred to forename use, derived from the English personal name Kayley, KEELEY means "slender."
Surname or Lastname
English and German
English and German : occupational name from Middle English, Middle Low German peller ‘maker (or seller) of expensive cloth’, derived from Old English pæll, pell ‘costly or purple cloth or cloak’, Middle Low German pelle (see Pelle 2).Southern English : topographic name for someone living by an inlet of the sea, a derivative of Old English pyll ‘inlet’ (see Pill 1) + the -er suffix denoting an inhabitant.German : from a Germanic personal name formed with bald ‘brave’ + heri ‘army’.
Surname or Lastname
English and Scottish
English and Scottish : topographic name, a variant of Sell 1.English and Scottish : occupational name for a saddler, from Anglo-Norman French seller (Old French sellier, Latin sellarius, a derivative of sella ‘seat’, ‘saddle’).English and Scottish : metonymic occupational name for someone employed in the cellars of a great house or monastery, from Anglo-Norman French celler ‘cellar’ (Old French cellier), or a reduction of the Middle English agent derivative cellerer.English and Scottish : occupational name for a tradesman or merchant, from an agent derivative of Middle English sell(en) ‘to sell’ (Old English sellan ‘to hand over, deliver’).German : probably a habitational name from a place named Sella near Hoyerswerda.
Male
English
Variant spelling of English unisex Kelly, KELLEY means "bright-headed."
Girl/Female
American, Australian, British, English
From the Pepper Plant; Hot Spice
Surname or Lastname
English and Scottish
English and Scottish : variant of Keillor.German : variant of Keller.
Male
Scottish
Medieval Scottish form of Latin Crescentius, KESTER means "to spring up, grow, thrive."
Boy/Male
British, Chinese, English
From the Pepper Plant
Surname or Lastname
German
German : from Middle High German kellaere ‘cellarman’, ‘cellar master’ (Latin cellarius, denoting the keeper of the cella ‘store chamber’, ‘pantry’). Hence an occupational name for the overseer of the stores, accounts, or household in general in, for example, a monastery or castle. Kellers were important as trusted stewards in a great household, and in some cases were promoted to ministerial rank. The surname is widespread throughout central Europe.English : either an occupational name for a maker of caps or cauls, from Middle English kellere, or an occupational name for an executioner, from Old English cwellere.Irish : reduced form of Kelleher.Scottish : variant of Keillor.
Surname or Lastname
English
English : occupational name for a boatman or boatbuilder, from an agent derivative of Middle English kele ‘ship’, ‘barge’ (from Middle Dutch kiel).Americanized spelling of German Kühler, from a variant of an old personal name (see Keeling) or a variant of Kuhl.
KEPLER PROBLEM
KEPLER PROBLEM
Girl/Female
American, Greek, Gujarati, Hindu, Indian
Grace; Favour; Pure
Girl/Female
Muslim
Wealth
Female
Norwegian
 Danish and Norwegian form of Latin Christina, KIRSTEN means "believer" or "follower of Christ." Compare with another form of Kirsten.
Boy/Male
Polish
Good/famous.
Boy/Male
Arabic, Muslim
Courier of the Truth (Allah)
Girl/Female
Indian, Telugu
A Deer
Girl/Female
Assamese, Bengali, Hindu, Indian, Malayalam, Marathi
Diamond; Beautiful Jewel
Boy/Male
Hindu
One name of God
Girl/Female
Arabic, Hawaiian, Hebrew
Born During Light; Nightfall
Boy/Male
Tamil
Huge and gigantic, The mighty one (Pandu and Kunti's second son, sired by Vayu, the wind-god. Bhima is described as a powerful, large and hugely strong man.)
KEPLER PROBLEM
KEPLER PROBLEM
KEPLER PROBLEM
KEPLER PROBLEM
KEPLER PROBLEM
a.
Having a median ridge; carinate; as, a keeled scale.
n.
See Kelter.
n.
The keeper of a pound.
n.
See Keeler, 1.
n.
See Replier.
n.
One who deals; one who has to do, or has concern, with others; esp., a trader, a trafficker, a shopkeeper, a broker, or a merchant; as, a dealer in dry goods; a dealer in stocks; a retail dealer.
n.
One employed in managing a Newcastle keel; -- called also keelman.
p. pr. & vb. n.
of Kipper
n.
One who tells stories; a narrator of anecdotes,incidents, or fictitious tales; as, an amusing story-teller.
n.
An apple seller; a hawker of, or dealer in, any kind of fruit or vegetables; a fruiterer.
n.
A small or shallow tub; esp., one used for holding materials for calking ships, or one used for washing dishes, etc.
n.
One who, or that which, helps, aids, assists, or relieves; as, a lay helper in a parish.
imp. & p. p.
of Kipper
n.
A fruit that keeps well; as, the Roxbury Russet is a good keeper.
n.
The plant which yields pepper, an East Indian woody climber (Piper nigrum), with ovate leaves and apetalous flowers in spikes opposite the leaves. The berries are red when ripe. Also, by extension, any one of the several hundred species of the genus Piper, widely dispersed throughout the tropical and subtropical regions of the earth.
n.
Any plant of the genus Capsicum, and its fruit; red pepper; as, the bell pepper.
n.
One who has the care, custody, or superintendence of anything; as, the keeper of a park, a pound, of sheep, of a gate, etc. ; the keeper of attached property; hence, one who saves from harm; a defender; a preserver.
v. t.
To sprinkle or season with pepper.
a.
Keel-shaped; having a longitudinal prominence on the back; as, a keeled leaf.