A star is formed from a Nebula (plural: nebulae). It is a cloud of dust and gas in Space. Some stars are formed at the same place where the previous star died. For example, a star explodes in supernova (such as supernova of Crab Nebula), the gasses and dust from the explosion remain behind that led to the birth of a new star.
Answer:
ω₂ = 13.09 rad/s
Explanation:
given,
small disk rotating speed = 500 rpm
radius of small disk = R
radius of larger disk = 2 R
rotational speed of larger disk = ?
using the law of conservation of angular momentum, we get
I₁ ω₁ = I₂ ω₂
moment of inertia for solid disk

now,
ω₂ = 125 rpm
and
ω₂ = 13.09 rad/s
the rotational speed of larger disc is equal to ω₂ = 13.09 rad/s
Answer:
-3.5 m/s²
Explanation:
- Initial Velocity = 21m /s
- Final velocity = 0m/s
- Distance = 63 m .
- Acclⁿ = ?
<u>We </u><u>know</u><u> </u><u>that</u><u> </u><u>:</u><u>-</u><u> </u>
Stopping distance = u²/2(-a)
63m = (21m/s)² / -2a
a = - 21 * 21 / 63 * 2 m/s²
a = - 3.5 m/s²
<em>*</em><em>*</em><em>Edits</em><em> </em><em>are</em><em> </em><em>welcomed</em><em>*</em><em>*</em>
Answer:
1.208
Explanation:
L = Length of tube
c = Speed of light in air
v = Speed of light in jelly
Time taken by light in tube

Time taken when jelly is present

Dividing the above equations we get

The refractive index of the jelly is 1.208
Answer:
I cant fit the entire picture but this should help