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11
The centre of gravity of a sprinter during the race lies
Discuss
Answer & Solution
Answer: Option A
Solution:
Running is a means of terrestrial locomotion allowing humans and other animals to move rapidly on foot. It is simply defined in athletics terms as a gait in which at regular points during the running cycle both feet are off the ground. This is in contrast to walking, where one foot is always in contact with the ground, the legs are kept mostly straight and the center of gravity vaults over the legs in an inverted pendulum fashion. A characteristic feature of a running body from the viewpoint of spring-mass mechanics is that changes in kinetic and potential energy within a stride occur simultaneously, with energy storage accomplished by springy tendons and passive muscle elasticity.
12
Who enunciated the laws of planetary motion?
Discuss
Answer & Solution
Answer: Option B
Solution:
Johannes Kepler published his first two laws about planetary motion in 1609 , having found them by analyzing the astronomical observations of Tycho Brahe. Kepler's third law was published in 1619.
13
The tidal waves on sea is mainly due to
Discuss
Answer & Solution
Answer: Option A
Solution:
The tidal waves on sea is mainly due to gravitational effect of Moon on Earth.
14
The time period of a pendulum when taken to the Moon would:
Discuss
Answer & Solution
Answer: Option D
Solution:
When the pendulum is taken to the moon, the value of 'g' will decrease and hence time period will increase. As the pendulum takes more time to complete one vibration, it will lose time.
15
"God Particle" is
Discuss
Answer & Solution
Answer: Option B
Solution:
"God Particle" is Higgs Boson.
16
The mass of a star is two times the mass of the Sun. How it will come to an end ?
Discuss
Answer & Solution
Answer: Option A
Solution:
The mass of a star which is two times the mass of the sun turns into a neutron star. A neutron star is a type of stellar remnant that can result from the gravitational collapse of a massive star during a Type II, Type Ib or Type Ic supernova event. Such stars are composed almost entirely of neutrons, which are subatomic particles without electrical charge and with slightly larger mass than protons. Neutron stars are very hot and are supported against further collapse by quantum degeneracy pressure due to the Pauli’s exclusion principle. This principle states that no two neutrons (or any other fermionic particles) can occupy the same place and quantum state simultaneously. A typical neutron star has a mass between about 1.4 and 3.2 solar masses ( Chandrasekhar Limit), with a corresponding radius of about 12 km if the Akmal– Pandharipande–Ravenhall equation of state (APR EOS) is used.
17
Which of the following celestial bodies contains abundant quantities of helium-3, a potential source of energy ?
Discuss
Answer & Solution
Answer: Option B
Solution:
The Moon has been bombarded with large quantities of Helium-3 by the solar wind.
18
The period of revolution of a certain planet in an orbit of radius R is T. Its period of revolution in an orbit of radius 4R will be:
Discuss
Answer & Solution
Answer: Option A
Solution:
The period of revolution of a certain planet in an orbit of radius R is T. Its period of revolution in an orbit of radius 4R will be 8T.
19
Which is evidence that supports the dynamo theory?
Discuss
Answer & Solution
Answer: Option B
Solution:
In physics, the dynamo theory proposes a mechanism by which a celestial body such as Earth or a star generates a magnetic field.
Earth's crust core contains a large amount of iron and nickel is the evidence of the dynamo theory.
20
Which of the following is indicated by the colour of a star ?
Discuss
Answer & Solution
Answer: Option C
Solution:
The color of a star mostly indicates a star's temperature, and it can also suggest the star's age. Class O stars, which are blue in color, are the hottest, and class M stars, which are red in color, are the coldest.