The magnifying power of an astronomical telescope will be:
"0.095".
According to the question,
Radius of curvature, R = 5.5 mm
Focal length of eyepiece, = 2.9 cm
We know that,
→ Focal length of mirror,
F₀ =
By substituting the values,
=
= 2.75 mm or,
= 0.278 cm
hence,
The telescope's magnification be:
=
=
= 0.095
Thus the above approach is correct.
Find out more information about magnification here:
Answer:
0.095
Explanation:
An astronomical telescope is a telescope used for viewing far distance object. It uses two lenses called the objective lens and the eyepiece lens.
Each lens has its own focal length
Let the focal length of the objective lens be Fo
Focal length of the eyepiece be Fe
Magnification of an astronomical telescope = Fo/Fe
Since the telescope uses a reflecting mirror having radius of curvature of 5.5mm instead of an objective lens, then we will replace Fo as the focal length of the mirror.
Focal length of a mirror Fo = Radius of curvature/2
Fo = R/2
Fo = 5.5/2
Fo = 2.75mm
Converting 2.75mm to cm gives 2.75/10 = 0.275cm
Fo = 0.275cm; Fe = 2.9cm
Magnification of the telescope = 0.275/2.9
Magnification of the astronomical telescope = 0.095
Answer:
Δ KE = - 8.75 x 10⁻⁴ J
Explanation:
given,
mass of applesauce = 7 g = 0.007 Kg
initial velocity, u = 0.5 m/s
final velocity, v = 0 m/s
Decrease in kinetic energy = ?
initial kinetic energy
KE₁ = 8.75 x 10⁻⁴ J
final kinetic energy
KE₂ =0 J
Decrease in kinetic energy
Δ KE = KE₂ - KE₁
Δ KE = 0 - 8.75 x 10⁻⁴
Δ KE = - 8.75 x 10⁻⁴ J
decrease in kinetic energy of the applesauce is equal to 8.75 x 10⁻⁴ J
The decrease in kinetic energy of the applesauce, when it hits the wall and stops, is the initial kinetic energy of it. Using the formula of kinetic energy, the decrease is calculated to be 0.000875 Joules.
This question relates to the concept of kinetic energy in physics. Kinetic energy is calculated by the formula 0.5 * mass (kg) * velocity (m/s)^2. So the initial kinetic energy of the applesauce right after being thrown was 0.5 * 0.007 kg * (0.5 m/s)^2 = 0.000875 Joules.
When the applesauce hits the wall and stops, its velocity drops to 0. Thus, its kinetic energy also goes to 0 (because kinetic energy is proportional to the square of velocity).
Therefore, the decrease in kinetic energy is the same as the initial kinetic energy of the applesauce, which is 0.000875 Joules.
#SPJ3
A. 926 m to the north
B. 5.2 m/s to the west
C. 46 m down
D. 12.3 m/s faster
Answer:
D is not the a vector quantities
Answer:
The underwater angles of refraction for the blue and red components of the light is 47.8° and 48.2°
Explanation:
Using the Snell's law
n1 * sin Ф1 = n2 sin Ф2
1 * sin 83 = n2 sin Ф2
Ф2 =
Red light
n2 = 1.331
Ф2 = °
Blue light
n2 = 1.340
Ф2 = °
Answer:
venus - 2
earth - 3
mars - 4
mercury - 1
Answer:
Speed of ball just before it hit the surface is 31.62 m/s .
Explanation:
Given :
Mass of ball , m = 50 g = 0.05 kg .
Height from which it falls , h = 80 m .
Thermal energy , E = 15 J .
Now , Initial energy of the system is :
Here , initial velocity is zero .
Therefore ,
Now , final energy of the system :
Since , no external force is applied .
Therefore , total energy of the system will be constant .
By conservation of energy :
Therefore , speed of ball just before it hit the surface is 31.62 m/s .
Using the principle of conservation of energy, the speed of the ball just before hitting the Earth's surface is found to be 79.2 m/s after accounting for the 15 J increase in thermal energy.
This question is concerned with the concept of conservation of energy, specifically the principles of potential and kinetic energy. When the ball is 80 meters above the Earth's surface, the total gravitational potential energy is m*g*h = 50g*9.8m/s²*80m = 39200 J (where m is mass, g is gravity, and h is height), and the kinetic energy is 0.
As the ball falls, its potential energy gets converted into kinetic energy, but we also know that the total thermal energy of the ball and the air in the system increases by 15 J. That means that not all the potential energy is converted into kinetic energy, 15 J is lost to thermal energy. So, the kinetic energy of the ball when it hits the Earth is 39200 J - 15 J = 39185 J.
Finally, we know that kinetic energy equals (1/2)*m*v², where v is the speed of the ball. Rearranging this formula to solve for v we get, v = sqrt((2*kinetic energy)/m) = sqrt((2*39185 J)/50g) = 79.2 m/s. So, just before the ball hits the surface, its speed is 79.2 m/s.
#SPJ12
Answer:
Work done will be equal to 3186.396 J
Explanation:
We have mass m = 76.2 kg
Initial velocity u = 5 m/sec
Final velocity v = 10.4 m/sec
We have to find the work done
From work energy theorem work done is equal to change in kinetic energy
w = 3168.396 J
So work done will be equal to 3186.396 J