Find the tangent line \(q\) to
the parabola \(4(y - 2) = (x + 1)^{2}\), so that the tangent \(q\)
is parallel to the line \(p\colon 4x - 5y + 17 = 0.\)
A body is thrown at the initial angle \(\alpha = 30^{\circ }\)
and the initial velocity \(v_{0} = 20\, \mathrm{m}/\mathrm{s}\).
The trajectory of the body is a part of parabola. Find the directrix of this
parabola. Hint: The coordinates of the moving body as functions of time are
\[
\begin{aligned}x& = v_{0}t\cdot \cos \alpha , &
\\y& = v_{0}t\cdot \sin \alpha -\frac{1}
{2}gt^{2}.
\\ \end{aligned}
\]
Consider the standard acceleration due to gravity
\(g = 10\, \mathrm{m}/\mathrm{s}^{2}\).
The Earth travels around the Sun on an elliptical orbit. The Sun is in the
focus of this ellipse. The maximal distance from Earth to the Sun is
\(152.1\cdot 10^{6}\, \mathrm{km}\), the minimal distance
from Earth to the Sun is \(147.1\cdot 10^{6}\, \mathrm{km}\).
Find the length of the semi-minor axis (one half of the length
of the shorter axis) and round your answer to the nearest
\(10^{4}\, \mathrm{km}\).
For an isothermal process in an ideal gas the product
\(pV \)
is constant (Boyle's law). In a pressure-volume diagram which shows
\(p\) as a
function of \(V \)
this law describes a hyperbola (called isotherm). Do we have enough information to
identify the asymptotes? If so, find these asymptotes.
On a map of a city, the town hall is represented by a point and a river through the
city by a straight line. There are places in the city with the property that the direct
distance from each place to the town hall is equal to the direct distance to the river.
In the following list identify a curve which can be used to join all these places.
Given physical quantities and laws relating these quantities, identify an answer
where the graph which relates these quantities is a part of a hyperbola. (The other
quantities are supposed to be constant.)
The pressure (\(p\)) and the
area (\(S\)) over which the
pressure is distributed, if \(F = p\cdot S\).
The mass (\(m\)) and
the kinetic energy (\(E_{k}\))
of a moving body, if \(E_{k} = \frac{1}
{2}\cdot m\cdot v^{2}\).
The velocity (\(v\)) and
the kinetic energy (\(E_{k}\))
of a moving body, if \(E_{k} = \frac{1}
{2}\cdot m\cdot v^{2}\).
The mass (\(m\)) and the potential
energy (\(E_{p}\)) in a homogeneous
gravitational field, if \(E_{p} = m\cdot g\cdot h\).