electromagnetic radiations
helium nuclei
negatively charged particles
neutral particles
B. helium nuclei
meteors
binaries
variable stars
bright stars
convex mirrors
concave mirrors
convex lens
concave lens
Voltmeter
Voltameter
Ammeter
Potentiometer
iron
chromium
copper
steel
proton
antiproton
positron
neutron
are good conductors of heat
are cheaper
are easily obtained
are bad conductors of heat
absorption of a neutron by a nucleus
breakup of the nucleus of a heavy atom into two nearly equal halves emitting two or three neutrons and releasing large amounts of nuclear energy in the process
the scattering of neutrons
formation of heavier nucleus
It will go down
It will come up
It will remain at the same level
First it will go down and it will come up
both pieces will lose their magnetism
one piece will have North Pole on both ends and the other South Pole on its both ends
each will remain a magnet with North Pole at one end and South Pole at the other
the longer piece will behave as a bar magnet while the smaller will have no magnetism at all
a horizontal position
a nearly vertical position with its South Pole downwards
a nearly vertical position with its North Pole downwards
a slanting position
diffusion
effusion
vaporisation
sublimation
greater
less
equal
can't be determined
linear motion
vibratory motion
rotational motion
None of the above
turbulence caused by the wind
buoyancy of air
unequal pressures acting on it
sudden change in the direction of the wind
increases
decreases
remains the same
first increases and then decreases
proton
neutron
electron
positron
Jupiter
Mars
Mercury
Saturn
is proportional to that of the Celsius thermometer
is always greater than that of the Celsius thermometer
is always less than that of the Celsius thermometer
may be greater than or less than or equal to that of the Celsius thermometer
Proxima Centauri
Sirius
Aldebaran
Vega
Rutherford
Bohr
Henri Bacquerel
Marie Curie
a planet
a meteor
a star
a comet
10-10 cm
10-12 cm
10-13 cm
10-16 cm
same number of protons but different number of neutrons
same number of neutrons but different number of protons
the same total number of protons and neutrons
same number of protons and different number of electrons
1
infinite
0
4
conservation of mass
Newtonian law of action and reaction
conservation of angular momentum
None of the above
a unit of time
a unit of length
a year of no consequence
illumination throughout the year
less than
greater than
equal to
greater than or equal to
Rutherford
Neils Bohr
Albert Einstein
JJ Thompson
inertia
adhesion
cohesion
friction
reverberate
be heard by us faintly
be heard upto 10 km from it
not be heard at any distance at all from it