Examples of using Angular distance in English and their translations into Spanish
{-}
-
Colloquial
-
Official
The planetary aspects or the angular distances between planets have a very….
The angular distance of the parhelia is depending on the elevation of the sun.
These coordinates are measured in degrees and represent angular distances… more.
Longitude- The angular distance east or west on the earth's surface.
The two brightest members of Alpha Librae are separated in the sky by an angular distance of 231" 3'51.
This allows the measure of angular distances between astronomical bodies.
This angular distance can be very small, but when you advance, the distance grows.
The amplitude of a saccade is the angular distance the eye travels during the movement.
By carefully measuring the position where theobjects were extinguished and knowing the focal length of the eyepiece, the angular distance could be calculated.
The latitude or angular distance between whichever point and the Equator, determines climates.
The linear blocks housing the living units divert from this knot creating angular distances between each other in an increasing level of privacy.
The height, or Elevation,is the angular distance of the horizon a point on the celestial sphere, measured as positive if facing the Zenith, and negative if directed towards the Nadir.
Given this precise distance measurement at the image plane,a trigonometric calculation with the objective focal length yields the angular distance between the two points seen in a telescope.
The real angular aspects,i.e. the real angular distances between planetary operators.
Blind persons whose visual acuity, as determined by competent authority, is 20/200 or less in the better eye with correcting lenses, orwhose widest diameter of visual field subtends an angular distance no greater than 20 degrees.
The heliographic longitude of a solar feature conventionally refers to its angular distance relative to the central meridian, i.e. that which the Sun-Earth line defines.
The Babylonian astronomers kept detailed records on the rising and setting of stars, the motion of the planets, and the solar and lunar eclipses,all of which required familiarity with angular distances measured on the celestial sphere.
The radial velocity of cluster members can be determined from Doppler shift measurements of their spectra, and once the radial velocity,proper motion and angular distance from the cluster to its vanishing point are known, simple trigonometry will reveal the distance to the cluster.
This represents a true technical challenge, as it requires combining the signals from all antennas and electronic components to produce a high-resolution image of the object under observation,with a precision of a millionth of a millionth of an arcsecond angular distance.
Each star had specific information recorded in columns: the reference number and magnitude found by astronomer Tycho Brahe, Johannes' own magnitude calculation, the star's longitude andlatitude by both ecliptic coordinates measured by angular distances and meridian altitudes found using Johannes' quadrant, and the star's equatorial coordinates calculated using spherical trigonometry.
The first ever micrometric screw was invented by William Gascoigne in the 17th century, as an enhancement of the vernier;it was used in a telescope to measure angular distances between stars and the relative sizes of celestial objects.
Linear size from angular size and distance Angular size.
PLANETCALC, Distance from angular size and linear size Comments.