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Carbon is the 4th most abundant element in the Universe

Carbon is the 4th most abundant element in the Universe.
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Recent Articles (Science Gallery)

OPTICAL-FIBRE-CABLE-LAYER
Researchers develop new method for detecting superfluid motion
S-Orbital
The Spectral Lines of Hydrogen Atom (3)
De Broglie Hypothesis (1)
Stern–Gerlach Experiment
Electric Field due to Circular loop of Charge
Electric Dipole Moment
Gauss Law
Compton Scattering
Miller Indices
Simple Cubic Crystal Structure
Helium-Neon Laser
Ruby Laser
Total Internal Reflection
Polarization of light
Exothermic & Endothermic Reaction
Faraday's Law of Induction
Body-Centered Cubic Unit Cell
“The body-centered cubic system has one lattice point in the center of the unit cell in addition to the eight corner points.”
DC Motor (1)
Interferometer
Davisson–Germer Experiment (5)
J.J. Thomson
In 1918, Max Planck awarded the Nobel Prize in Physics for the Discovery of Energy Quanta.
The photoelectric effect
Simple Machines - Levers
Structure of The Earth
Visible Light Spectrum
Energy band diagram
Layers of the Atmosphere
Double Slit Experiment (1)
Carl David Anderson (2)
Braggs law
Multiverse
pentaquark
Composition-of-Air
Buoyant-Force
hookes law
sound space
Wormhole
A-day-on-Venus-is-longer-than-a-year
water waves
tetra quark
Tunnel diode
Quantum Dots
Quantum Teleportation: Fundamentals and Visualizations
A Windmill is a Machine that converts Wind Energy into Rotational Energy and then Rotational Energy into Electrical Energy.
A day on a Venus is Longer Than a Year (1)
Why You Can’t Hear Sound in Space? Because sound does not travel in space. Sound is just a vibration of air or sound is just travel through the vibration of atoms and molecules. Because, Space is vacuum or empty, there is no medium of travel for sound.
Gravitational wave
Why Space is Black
If Light Has No Mass, then why is It Affected by Black Holes
What is a brown dwarf? Explained
Carbon is the 4th most abundant element in the Universe.
Magnetic Bearing
Light Emitting Diode
Inside Planet Mars
temperature variation on the surface of planet mercury
Saturn
SpaceTime
Wilberforce Pendulum
Absorption (electromagnetic radiation)
Meissner effect
Magnetic refrigeration
Phase Transitions Diagram
Meissner effect
Categorizing Different lighting with Temperatures

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Lens aberration

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The "Four Pillars" of the Big Bang Theory

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Elliptical Galaxies

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Time Dilation
Neutron Star

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Standard model of particle physics

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Helium

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Ohm's law was Probably the most Important of the Early Quantitative descriptions of the Physics of Electricity

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Superfluidity

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