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Can two lines with the same x intercept be perpendiclar?
In 2-dimensions, the answer is No. Unless the x-axis is counted as having an infinite number of intercepts with itself. In more than 2-dimensions, the answer is Yes.
How are perpendiclar lines different from intersecting lines?
Perpendicular lines are those that even if stretched to infinite lengths, they will NEVER touch. Intersecting lines are those that aren't necessarily 90 degres seperated, but ones that will, at one point, cross over.
What is the base of the triangular prism?
well there are three rectangles and 2 triangles so it could be either a rectangle or a triangle!!!! Helen Prism is a body, formed by extruding a given area in a plane perpendiclar to that plan which consists the give area. In case of triangular prism, triangle is stretched to form a volume. It includes two triangles with threee rectangles. Either of triangle can be treated as base of the prism.
What is the perpendiclar sides in a right triangle?
It is where the 90 degree angle is located.
How many perpendiclar lines does a pentagon have?
None, since there are no right angles in a pentagon. The angles are 360/5 = 72o
Can two lines with the same x intercept be perpendiclar?
In 2-dimensions, the answer is No. Unless the x-axis is counted as having an infinite number of intercepts with itself. In more than 2-dimensions, the answer is Yes.
Triangle ABc has right angle which is angle ABC and a line is formed called line segment abd draw this figure in order to solve problem below if line segment ac is perpendiclar to linesegment cb an?
35 degrees
How are perpendiclar lines different from intersecting lines?
Perpendicular lines are those that even if stretched to infinite lengths, they will NEVER touch. Intersecting lines are those that aren't necessarily 90 degres seperated, but ones that will, at one point, cross over.
What is the base of the triangular prism?
well there are three rectangles and 2 triangles so it could be either a rectangle or a triangle!!!! Helen Prism is a body, formed by extruding a given area in a plane perpendiclar to that plan which consists the give area. In case of triangular prism, triangle is stretched to form a volume. It includes two triangles with threee rectangles. Either of triangle can be treated as base of the prism.
What wave occur when the motion of medium is at right angels ( perpendiclar) to the direction of th e wave?
Transverse waves occur when the particles of the medium move perpendicular to the direction of the wave. This motion creates crests and troughs as the energy is transferred perpendicular to the direction of the wave propagation. Examples of transverse waves include light waves and electromagnetic waves.
What is spectrograph test?
The procedure that has been adopted for the processing of the data includes the following stages:The spectrum of a reference star is obtained.The sky is removed from the raw spectral star image.The columns perpendiclar to the spectral image are added to obtain the stella spectrum.These tasks have been performed in IRIS. The sky removal and optimal addition options within IRIS both seem to give excellent results.The output from IRIS has had the local sky effects removed but is still dependant on the spectral response of the optical system. To calibrate the spectrum we do the following:Divide our spectrum by a library spectrum for the same spectral type.The resulting curve is smoothed.This is then used to calibrate the other spectra... We divide our other spectra by the calibration curve.These tasks are performed in Visual Spec. The library spectra are supplied as part of that package. These appear to be from the Pickles catalogue and are normalised with to 550nm (V-Band) to equal a relative flux value of 1.It is clear that errors could be included at each step in the procedure. It would also be very complex to calculate these individual errors. However, the differences between the different spectra of the same star taken over the course of a number of nights would give us a good idea of the overall accuracy of our results.So.... If we.....Take the spectrum of a reference star, process it to obtain a spectral response curve.Take the spectrum of another star with a different spectral type, use the response curve to calibrate it.Repeat this same procedure a number of times over a number of different nights.Compare the data sets and calculate an error value for each wavelength and hopefully a percentage error.Convert this to an average error across the B, V & R bands if this is possible.This could then provide some level of quality assurance for the spectra obtained.I hope it help you... :)
