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In geometry, an axis-aligned object (axis-parallel, axis-oriented) is an object in n-dimensional space whose shape is aligned with the coordinate axes
Axis-aligned_object
Smallest box which encloses some set of points
coordinate for the points in S. Axis-aligned minimal bounding boxes are used as an approximate location of an object in question and as a very simple
Minimum_bounding_box
A rigid body with 3 distinct axes of inertia is unstable rotating about the middle axis
rotation of an object around its first and third principal axes is stable, whereas rotation around its second principal axis (or intermediate axis) is not.
Tennis_racket_theorem
Solar system objects beyond the other known trans-Neptunian objects
trans-Neptunian object (ETNO) orbits are suspected to be aligned with the hypothetical Planet Nine while the blue-colored ETNO orbits are anti-aligned. The highly
Extreme trans-Neptunian object
Extreme_trans-Neptunian_object
Hypothetical Solar System planet
alignment also switched, from more aligned to anti-aligned with increasing semi-major axis, and from anti-aligned to aligned with increasing perihelion distance
Planet_Nine
vary with semi-major axis of the object and if the object is in resonance. At smaller semi-major axes the aligned and anti-aligned regions shrink and eventually
Effects of Planet Nine on trans-Neptunian objects
Effects_of_Planet_Nine_on_trans-Neptunian_objects
Scalar measure of the rotational inertia with respect to a fixed axis of rotation
\end{aligned}}} Here I x x {\displaystyle I_{xx}} denotes the moment of inertia around the x {\displaystyle x} -axis when the objects are rotated
Moment_of_inertia
Movement of an object which leaves at least one point unchanged
perpendicular to that axis). Similarly, the rotation rate of an object in three dimensions at any instant is about some axis, although this axis may be changing
Rotation
Type of motion
kinetic energy of the object, and for the forces on the parts of the object, are also simpler for rotation around a fixed axis, than for general rotational
Rotation_around_a_fixed_axis
Polygon in which all angles are right
iso-oriented, axis-aligned, and axis-oriented polygons. These adjectives are less confusing when the polygons of this type are rectangles, and the term axis-aligned
Rectilinear_polygon
Term in geometry; longest and shortest semidiameters of an ellipse
{\displaystyle {\begin{aligned}b&=a{\sqrt {1-e^{2}}},\\\ell &=a(1-e^{2}),\\a\ell &=b^{2}.\end{aligned}}} The semi-major axis of a hyperbola is, depending
Semi-major and semi-minor axes
Semi-major_and_semi-minor_axes
Mounting system for camera or telescope
instrument attached to it to stay fixed on any celestial object with diurnal motion by driving one axis at a constant speed. Such an arrangement is called a
Equatorial_mount
Optical imaging rule
image and object distances, so that m = − v u = − v − f f . {\displaystyle {\begin{aligned}m&=-{\frac {v}{u}}\\&=-{\frac {v-f}{f}}.\end{aligned}}} On the
Scheimpflug_principle
Type of motion which combines translation and rotation with respect to a surface
in the object axis is a line, while the trajectory of any point in the object rim is a cycloid. The velocity of any point in the rolling object is given
Rolling
Celestial coordinate system used to specify the positions of celestial objects
+ X η = y + Y ζ = z + Z {\displaystyle {\begin{aligned}\xi &=x+X\\\eta &=y+Y\\\zeta &=z+Z\end{aligned}}} Celestial coordinate system Planetary coordinate
Equatorial_coordinate_system
Design technique
three-dimensional object (3D object) on a two-dimensional plane. These projections rely on visual perspective and aspect analysis to project a complex object for viewing
3D_projection
Major alliance of World War II
The Axis powers, originally called the Rome–Berlin Axis and later, the Rome–Berlin–Tokyo Axis, was the military coalition which initiated World War II
Axis_powers
Theorem in planar dynamics
of area of a rigid body about any axis, given the body's moment of inertia about a parallel axis through the object's center of gravity and the perpendicular
Parallel_axis_theorem
Coordinate system using perpendicular axes
{\displaystyle {\begin{aligned}(+x,+y,+z)&&(-x,+y,+z)&&(+x,-y,+z)&&(+x,+y,-z)\\(+x,-y,-z)&&(-x,+y,-z)&&(-x,-y,+z)&&(-x,-y,-z)\end{aligned}}} The coordinates
Cartesian_coordinate_system
Graph of space and time in special relativity
horizontal axis and time on the vertical axis. Additionally, the time and space units of measurement are chosen in such a way that an object moving at
Spacetime_diagram
Object movement along a circular path
In kinematics, circular motion is the motion of an object along a circular path. Examples of this include a stone tied to a string, a car moving around
Circular_motion
Mathematical construct in engineering
{\displaystyle J} (for an axis perpendicular to the plane). In both cases, it is calculated with a multiple integral over the object in question. Its dimension
Second_moment_of_area
Type of inertial force
appears to act on all objects when viewed in a rotating frame of reference. It appears to be directed perpendicularly from the axis of rotation of the frame
Centrifugal_force
Loss of one degree of freedom in a three-dimensional, three-gimbal mechanism
accommodate rotation about one axis, leaving the suspended object effectively locked (i.e. unable to rotate) around that axis. The problem can be generalized
Gimbal_lock
Periodic change in the direction of a rotation axis
symmetry axis. When an object is not perfectly rigid, inelastic dissipation will tend to damp torque-free precession, and the rotation axis will align itself
Precession
Conserved physical quantity; rotational analogue of linear momentum
{\begin{aligned}\mathbf {r} _{i}&=\mathbf {v} _{i}=\mathbf {0} ,\\\mathbf {r} &=\mathbf {R} ,\\\mathbf {v} &=\mathbf {V} ,\\m&=M,\end{aligned}}} ∑ i r
Angular_momentum
Straight figure with zero width and depth
{\displaystyle {\begin{aligned}X&=(x_{1},x_{2},\dots ,x_{n}),\\Y&=(y_{1},y_{2},\dots ,y_{n}),\\Z&=(z_{1},z_{2},\dots ,z_{n}),\end{aligned}}} are collinear if
Line_(geometry)
Curved path of an object around a point
an object under the influence of an attracting force. Alternatively, it is known as an orbital revolution, because it is a rotation around an axis external
Orbit
Lens with a thickness that is negligible
{\begin{aligned}e&\approx nr_{2}\\&=n(i-r_{1})\\&\approx n(i-{\frac {i}{n}})\end{aligned}}} If the incoming ray is parallel to the optical axis and distance
Thin_lens
Position of something in relation to its surroundings
similar method, called axis–angle representation, describes a rotation or orientation using a unit vector aligned with the rotation axis, and a separate value
Orientation_(geometry)
Visible star that is nearly aligned with Earth's axis of rotation
A pole star is a visible star that is approximately aligned with the axis of rotation of an astronomical body; that is, a star whose apparent position
Pole_star
Method for visually representing three-dimensional objects
with the camera aligned parallel to the floor and aligned to the coordinate axes, it is first rotated horizontally (around the vertical axis) by ±45°, then
Isometric_projection
Six points which determine imaging properties of an optical system
centred on the optical axis there will only pass rays that were emitted from the object at a sufficiently small angle from the optical axis. Using a sufficiently
Cardinal_point_(optics)
Variance in a celestial body's axis of rotation over time
a phenomenon which causes the orientation of the axis of rotation of a spinning astronomical object to vary over time. It is caused by the gravitational
Astronomical_nutation
Optical device which transmits and refracts light
material), u {\textstyle u} is the on-axis (on the optical axis) object distance from the line perpendicular to the axis toward the refraction point on the
Lens
Area of the Solar System beyond the planets, comprising small bodies
corresponds to a characteristic semi-major axis of about 39.4 AU. This 2:3 resonance is populated by about 200 known objects, including Pluto together with its
Kuiper_belt
Time-telling device
the geographical latitude. This axis is aligned with the celestial poles, which is closely, but not perfectly, aligned with the pole star Polaris. For
Sundial
Number of rotations per unit time
lowercase Greek nu, and also n), is the frequency of rotation of an object around an axis. Its SI unit is the reciprocal seconds (s−1); other common units
Rotational_frequency
Geometric objects with a common centre
quadrics. Geometric objects are coaxial if they share the same axis (line of symmetry). Geometric objects with a well-defined axis include circles (any
Concentric_objects
Speed and direction of a motion
{u}})+a^{2}t^{2}\end{aligned}}} ( 2 a ) ⋅ x = ( 2 a ) ⋅ ( u t + 1 2 a t 2 ) = 2 t ( a ⋅ u ) + a 2 t 2 = v 2 − u 2 {\displaystyle {\begin{aligned}(2{\boldsymbol
Velocity
Representation of a curve by a function of a parameter
parametrisation) of the object. For example, the equations x = cos t y = sin t {\displaystyle {\begin{aligned}x&=\cos t\\y&=\sin t\end{aligned}}} form a parametric
Parametric_equation
Coordinates comprising a distance and two angles
{\displaystyle {\begin{aligned}x&=r\sin \theta \,\cos \varphi ,\\y&=r\sin \theta \,\sin \varphi ,\\z&=r\cos \theta .\end{aligned}}} Cylindrical coordinates
Spherical_coordinate_system
Movement of an object which leaves one point unchanged
cos θ . {\displaystyle {\begin{aligned}x'&=x\cos \theta -y\sin \theta \\y'&=x\sin \theta +y\cos \theta .\end{aligned}}} The vectors [ x y ] {\displaystyle
2D_rotation
Geometric civil engineering calculation technique
{MPa}}\\\end{aligned}}} σ 2 = σ a v g − R = − 30 MPa {\displaystyle {\begin{aligned}\sigma _{2}&=\sigma _{\mathrm {avg} }-R\\&=-30{\textrm {MPa}}\\\end{aligned}}}
Mohr's_circle
Correspondence between quaternions and 3D rotations
+\alpha }{2}}\right)\mathbf {B} \times \mathbf {A} \end{aligned}}} finally normalizing the rotation axis: D 2 sin 1 2 γ {\textstyle {\frac {\mathbf {D} }{2\sin
Quaternions and spatial rotation
Quaternions_and_spatial_rotation
Description of the orientation of a rigid body
the object. As an example, consider a top. If we define the Z axis to be the symmetry axis of the top, then the top spinning around its own axis of symmetry
Euler_angles
Design rule for optical systems
optical system in order for it to produce sharp images of off-axis as well as on-axis objects. It was formulated by Ernst Abbe in the context of microscopes
Abbe_sine_condition
Celestial coordinate system used to describe Solar System objects
z = r sin b {\displaystyle {\begin{aligned}x&=r\cos b\cos \ell \\y&=r\cos b\sin \ell \\z&=r\sin b\end{aligned}}} [ x equatorial y equatorial z equatorial
Ecliptic_coordinate_system
Constraint equations of a mechanical system
t\end{aligned}}.} In programming, this is often performed with the algorithm, x ← x + v t + 1 2 a t 2 v ← v + a t . {\displaystyle {\begin{aligned}\mathbf
Kinematics_equations
Apparent force in a rotating reference frame
proportional to the object's speed in the rotating frame (more precisely, to the component of its velocity that is perpendicular to the axis of rotation). The
Coriolis_force
Apparent unusual observation in the sky
An unidentified flying object (UFO) is an object or phenomenon seen in the sky but not yet identified or explained. The term was coined when United States
Unidentified_flying_object
Closed volume that completely contains the union of a set of objects
object. In most applications the axis of the cylinder is aligned with the vertical direction of the scene. Cylinders are appropriate for 3-D objects that
Bounding_volume
Family of linear transformations
{\displaystyle {\begin{aligned}t'&=\gamma \left(t-{\frac {vx}{c^{2}}}\right)\\x'&=\gamma \left(x-vt\right)\\y'&=y\\z'&=z\end{aligned}}} where (t, x, y, z)
Lorentz_transformation
Process of enlarging the apparent size of something
subtended by an object (w.r.t the optical axis) and ε {\textstyle \varepsilon } is the angle subtended by its image (also w.r.t the optical axis) made by an
Magnification
Coordinates comprising two distances and an angle
ρ sin φ z = z {\displaystyle {\begin{aligned}x&=\rho \cos \varphi \\y&=\rho \sin \varphi \\z&=z\end{aligned}}} in one direction, and ρ = x 2 + y 2 φ
Cylindrical_coordinate_system
Rate of change of velocity
{\displaystyle {\begin{aligned}a_{x}&={\frac {dv_{x}}{dt}}={\frac {d^{2}x}{dt^{2}}},\\a_{y}&={\frac {dv_{y}}{dt}}={\frac {d^{2}y}{dt^{2}}}.\end{aligned}}} The two-dimensional
Acceleration
Group of rotations in 3 dimensions
2 , {\displaystyle {\begin{aligned}q&=w+x\mathbf {i} +y\mathbf {j} +z\mathbf {k} ,\\1&=w^{2}+x^{2}+y^{2}+z^{2},\end{aligned}}} is mapped to the rotation
3D_rotation_group
Geometric method for visualizing a rotating rigid body
intermediate axis is not aligned with the angular momentum, then the podhode will be a curbe going from one end of the intermediate axis to the other
Poinsot's_ellipsoid
Coordinate frames
J2000 or EME2000. The x-axis is aligned with the mean vernal equinox. The z-axis is aligned with the Earth's rotation axis (or equivalently, the celestial
Earth-centered_inertial
Measure of how closely the shape of an object approaches that of a circle
points on the object, but is a separate precision bearing usually on the measuring instrument. The axis of the object or part of the object to be measured
Roundness
Surface formed by rotating an ellipse
{\begin{aligned}e&={\sqrt {2f-f^{2}}}\\f&=1-{\sqrt {1-e^{2}}}\end{aligned}}} All modern geodetic ellipsoids are defined by the semi-major axis plus either
Spheroid
Method of orienting telescopes and other celestial observation devices
the act of aligning the rotational axis of a telescope's equatorial mount or a sundial's gnomon with a celestial pole to parallel Earth's axis. The method
Polar_alignment
Small patches of nebulosity associated with newly born stars
Herbig–Haro objects are commonly found in star-forming regions, and several are often seen around a single star, aligned with its rotational axis. Most of
Herbig–Haro_object
Optical aberration
i + o , {\displaystyle {\begin{aligned}s&={\frac {R_{2}+R_{1}}{R_{2}-R_{1}}}\\[8pt]p&={\frac {i-o}{i+o}},\end{aligned}}} one can write the longitudinal
Spherical_aberration
superset, BSP trees). Finally, BIH is axis-aligned as are its ancestors. Although a more general non-axis-aligned implementation of the BIH should be possible
Bounding_interval_hierarchy
Kuiper belt object, not controlled by an orbital resonance with Neptune
traditional usage of the terms is based on the orbit's semi-major axis, and includes objects situated between the 2:3 and 1:2 resonances, that is between 39
Classical_Kuiper_belt_object
Device to facilitate robotic insertion into holes with tight clearance
peg over the hole, and then push the peg along the axis of the hole. If the peg is perfectly aligned and centered, it would then slide into the hole. However
Remote_center_compliance
Turning force around an axis
body, a torque can be thought of as a twist applied to an object with respect to a chosen axis. For example, when driving a screw, a screwdriver applies
Torque
System for specifying positions of celestial objects
own axis once per sidereal day (23 hours, 56 minutes and 4.091 seconds) in relation to the star background. The positioning of a celestial object by the
Astronomical coordinate systems
Astronomical_coordinate_systems
Limiting case which is different from the rest of the class
lower-dimensional hyperrectangle, all the way down to a point if the sides aligned with every axis have length zero. A convex polygon is degenerate if at least two
Degeneracy_(mathematics)
Distant body in the outer Solar System
its semi-major axis to the 3/2 power, times a constant 1.7×1016.(see equation 4) If an object's Λ is greater than 1, then that object will eventually
Sedna_(dwarf_planet)
Diagnostic instrument used to assess the extent and axis of astigmatism
4 apertures – As there are two prisms, each aligned perpendicular to the other, the major and minor axis powers can be measured independently without
Keratometer
Energy of a moving physical body
an axis through the center of mass and the rotation measured by ω must be around that axis; more general equations exist for systems where the object is
Kinetic_energy
Frame-dependent apparent force in Physics
apparent change in the velocity of an object when its position changes, putting it nearer to or further from the axis of rotation (the change in ∑ x j d
Fictitious_force
frame, with X-axis aligned to the south, where the local meridian intersects the horizon, Y-axis toward the eastern horizon, and Z-axis toward the zenith
Parallactic_angle
Equation for the velocity of a body in viscous fluid
z–axis is through the centre of the sphere and aligned with the mean flow direction, while r is the radius as measured perpendicular to the z–axis. The
Stokes's_law
Equations that describe the behavior of a physical system
_{0}\,,&[2]\\\end{aligned}}} in magnitudes, v = a t + v 0 , [ 1 ] r = a t 2 2 + v 0 t + r 0 . [ 2 ] {\displaystyle {\begin{aligned}v&=at+v_{0}\,,&[1]\\r&={\frac
Equations_of_motion
Estimation of orbits of objects
orbiting objects. As time goes by, the actual path of an orbiting object tends to diverge from the predicted path (especially if the object is subject
Orbit_determination
Sednoid
2023 KQ14, informally nicknamed Ammonite, is a trans-Neptunian object (TNO) orbiting the Sun on an extremely wide elliptical orbit. It was discovered by
2023_KQ14
Stream of ionized matter flowing away from a rotating astronomical object
velocity from an astronomical object, in a pair of narrow streams in opposite directions, aligned with the object's axis of rotation. When the matter in
Astrophysical_jet
Visual illusion of 3D scene
intelligible icons which represent objects or concepts. In this autostereogram, patterns become smaller and smaller down the y-axis, until they look like random
Autostereogram
Celestial coordinate system in spherical coordinates, with the Sun as its center
velocities of galactic objects. In these systems the xyz-axes are designated UVW, but the definitions vary by author. In one system, the U axis is directed toward
Galactic_coordinate_system
Defining the orbit of an object in space
ascending node, is one of the orbital elements used to specify the orbit of an object in space. Denoted with the symbol Ω, it is the angle from a specified reference
Longitude of the ascending node
Longitude_of_the_ascending_node
Topics referred to by the same term
star, a visible star approximately aligned with a celestial pole Geographical pole, two points on Earth where its axis of rotation intersects its surface
Pole
Physical phenomenon
following is valid: objects that are at rest on the surface of the Earth, co-rotating with the Earth, are circling the Earth's axis, so they are in centripetal
Eötvös_effect
Center of mass of multiple bodies orbiting each other
or more bodies orbit. A barycenter is a dynamical point, not a physical object. It is an important concept in fields such as astronomy and astrophysics
Barycenter_(astronomy)
Angle between a reference plane and the plane of an orbit
the tilt of an object's orbit around a celestial body. It is expressed as the angle between a reference plane and the orbital plane or axis of direction
Orbital_inclination
Measure of relativistic velocity
p | = γ m v . {\displaystyle {\begin{aligned}E&=\gamma mc^{2}\\\left|\mathbf {p} \right|&=\gamma mv.\end{aligned}}} With the definition of w w = artanh
Rapidity
Spiral with constant distance from itself
Archimedean spirals. Suppose a point object moves in the Cartesian system with a constant velocity v directed parallel to the x-axis, with respect to the xy-plane
Archimedean_spiral
Doughnut-shaped surface of revolution
{\begin{aligned}A&=\left(2\pi r\right)\left(2\pi R\right)=4\pi ^{2}Rr,\\[5mu]V&=\left(\pi r^{2}\right)\left(2\pi R\right)=2\pi ^{2}Rr^{2}.\end{aligned}}} These
Torus
Horizontal angle from north or other reference cardinal direction
1 + D cos α {\displaystyle {\begin{aligned}X_{2}&=X_{1}+D\sin \alpha \\Y_{2}&=Y_{1}+D\cos \alpha \end{aligned}}} This is typically used in triangulation
Azimuth
Interface in computer science, human-computer interaction, and interaction design
three arrows translates the object along the appropriate axis. The axes may be aligned with the world-space axes, the object-space axes, or some other space
Direct_manipulation_interface
Type of telescope mount and related software
coordinates. To track the object so that it stays in the eyepiece despite Earth's rotation, only the right-ascension axis is moved. Smart telescopes
GoTo_(telescopes)
Plane curve: conic section
{\displaystyle {\begin{aligned}h&={\frac {p}{2}},\\q&={\sqrt {f^{2}+h^{2}}},\\s&={\frac {hq}{f}}+f\ln {\frac {h+q}{f}}.\end{aligned}}} This quantity s is
Parabola
Device that orients a payload towards the Sun
side. Thus according to the above table, an optimally aligned single-axis tracker (see polar aligned tracker below) will only lose 8.3% at the summer and
Solar_tracker
Branch of mathematics that studies the properties of groups
{\displaystyle {\begin{aligned}\sum _{n\geq 1}{\frac {1}{n^{s}}}&=\prod _{p{\text{ prime}}}{\frac {1}{1-p^{-s}}},\\\end{aligned}}\!} captures the fact
Group_theory
3D model's surface projected to a 2D image
P} to the sphere's origin. Assuming that the sphere's poles are aligned with the Y axis, UV coordinates in the range [ 0 , 1 ] {\displaystyle [0,1]} can
UV_mapping
Techniques used to reduce blurring of images
electronic image stabilization can also compensate for rotation about the optical axis (roll). It is mainly used in high-end image-stabilized binoculars, still
Image_stabilization
Three-dimensional solid
a = r sin α . {\displaystyle {\begin{aligned}e&=\cos \alpha ,\\[1ex]a&={\frac {r}{\sin \alpha }}.\end{aligned}}} If the base of a circular cylinder has
Cylinder
Ways to represent 3D rotations
1-2\left(q_{j}^{2}+q_{k}^{2}\right)\right)\end{aligned}}} Given the Euler axis ê and angle θ, the quaternion q = [ q i q j q k q r ] = q i
Rotation formulations in three dimensions
Rotation_formulations_in_three_dimensions
AXIS ALIGNED-OBJECT
AXIS ALIGNED-OBJECT
Boy/Male
Indian, Sanskrit
Axis; Yoke
Boy/Male
Egyptian
Apis.
Female
English
 Short form of English Alisa, ALIS means "noble sort." Compare with another form of Alis.
Surname or Lastname
English
English : from the Norman female personal name Avice (Old French Avice, Latin Avitia, also found in a masculine form, Avitius). This is of uncertain origin, perhaps from a Celtic (Gaulish) name.French : Tanguay and Jetté have people named Avice, Avisse in Quebec from 1666. Nègre has an Avèze (Puy-de-Dome) also deriving from Avitius.
Female
English
 English adopted use of German Avis ("refuge in war"). But its popularity in the Middle Ages was due to its association with the Latin noun avis, AVIS means "bird."Â
Girl/Female
Assamese, Indian
Tall; Pivot; Pole; Axis
Girl/Female
Indian
Blessing, Prayer
Boy/Male
Egyptian
Mythical dead bull thought to be Osiris.
Male
Egyptian
, Apis.
Female
German
 Old German nickname, possibly AVIS means "refuge in war." Compare with another form of Avis.
Boy/Male
Muslim
Pivot. Pole. Axis. Celebrity.
Surname or Lastname
English
English : variant of Ames.
Boy/Male
Muslim
Companion. Genial. Close friend.
Boy/Male
Muslim
Pivot. Pole. Axis. Celebrity.
Girl/Female
Indian
Axis
Boy/Male
Arabic, Muslim
Pivot; Pole; Axis; Celebrity; Personality
Boy/Male
Indian
Close friend, Good company, Smart one, Companion, Supreme
Female
Welsh
 Welsh form of French Alais, ALIS means "noble sort." Compare with another form of Alis.
Female
French
 Contracted form of French Adeline, ALINE means "little noble." Compare with another form of Aline.
Female
English
 Variant spelling of English Aileen, ALINE means "little Eve." Compare with another form of Aline.
AXIS ALIGNED-OBJECT
AXIS ALIGNED-OBJECT
Boy/Male
Biblical
Desolation, destruction.
Girl/Female
Hindu, Indian
Sweet Basil
Girl/Female
Spanish American
Sorrow. From Maria de los Dolores (the Virgin Mary, or Mary of the Sorrows). Famous Bearer: the...
Boy/Male
Muslim
The guide to the right path
Boy/Male
African
youth'.
Girl/Female
Indian, Telugu
Moon Light
Girl/Female
Hindu
Princess
Boy/Male
Australian, Danish, German, Swedish
Brave with the Spear; Spear Rule
Girl/Female
Hindu
Good luck, Auspicious
Girl/Female
Afghan, American, Arabic, Celebrity, Farsi, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Muslim, Oriya, Pashtun, Punjabi, Sanskrit, Sikh, Sindhi, Tamil
Woman; Life; Small One; Simple; Successes; Wife of Prophet
AXIS ALIGNED-OBJECT
AXIS ALIGNED-OBJECT
AXIS ALIGNED-OBJECT
AXIS ALIGNED-OBJECT
AXIS ALIGNED-OBJECT
imp. & p. p.
of Malign
n.
The primary or secondary central line of any design.
n.
The space between two axes. See Axis, 6.
v. t.
To adjust or form to a line; to range or form in line; to bring into line; to aline.
n.
A straight line with respect to which the different parts of a magnitude are symmetrically arranged; as, the axis of a cylinder, i. e., the axis of a cone, that is, the straight line joining the vertex and the center of the base; the axis of a circle, any straight line passing through the center.
n.
Also used of the body only of the vertebra, which is prolonged anteriorly within the foramen of the first vertebra or atlas, so as to form the odontoid process or peg which serves as a pivot for the atlas and head to turn upon.
a.
Formed by right lines; rectilineal; as, a right-lined angle.
a.
Revolving on an axis.
n.
See Axis cylinder, under Axis.
v. t.
To alien or alienate; to transfer, as title or property; as, to aliene an estate.
n.
The spotted deer (Cervus axis or Axis maculata) of India, where it is called hog deer and parrah (Moorish name).
n.
The second vertebra of the neck, or vertebra dentata.
adv. & a.
From another source; from elsewhere; as, a case proved aliunde; evidence aliunde.
n.
One of several imaginary lines, assumed in describing the position of the planes by which a crystal is bounded.
n.
A genus of insects of the order Hymenoptera, including the common honeybee (Apis mellifica) and other related species. See Honeybee.
a.
Of or pertaining to an axis; of the nature of, or resembling, an axis; around an axis.
pl.
of Axis
n.
A straight line, real or imaginary, passing through a body, on which it revolves, or may be supposed to revolve; a line passing through a body or system around which the parts are symmetrically arranged.
v. t.
To range or place in a line; to bring into line; to align.
n.
The stem; the central part, or longitudinal support, on which organs or parts are arranged; the central line of any body.