Answer:
ω₂ = 1.9025 x 10⁻⁶ rad/s
Explanation:
given,
mass of star = 1.61 x 10³¹ kg
angular velocity = 1.60 x 10⁻⁷ rad/s
diameter suddenly shrinks = 0.29 x present size
r₂ = 0.29 r₁
using conservation of angular momentum
I₁ ω₁ = I₂ ω₂





ω₂ = 1.9025 x 10⁻⁶ rad/s
Answer:within the focal length of the lens, provided the focal length is shorter than the near point distance.
Explanation:Hope it helps
Answer:
To summarize, <em><u>Jane's star</u></em> has a <em><u>red</u></em> light and <em><u>is traveling towards</u></em> the <em><u>Earth</u></em> while <em><u>John's star </u></em>has a <em><u>blue</u></em> light and <em><u>is traveling away</u></em> from the <em><u>Earth</u></em>. This is a <em><u>prime example</u></em> of the <em><u>Doppler Effect</u></em> in <em><u>motion</u></em>. The stars <em><u>look different </u></em>because <em><u>they are traveling in different directions.</u></em>
Answer:
Explanation:
At the temperature of 1000K , hydrogen will have following degree of freedom
translational = 3
rotational = 2
vibrational = 1
Total = 6
Internal energy = 6N x 1 /2 k T where N is no of molecules
E₁ = 3 N kT
At the temperature of 1000K , helium will have following degree of freedom
translational = 3
rotational = 0
vibrational = 0
Total = 3
Internal energy = 3N x 1 /2 k T where N is no of molecules
E₂ = 3 / 2 N kT
Ratio = E₁ / E₂
= 2