EV_001neutral
Sunlight reaches Earth's atmosphere and is scattered in all directions by all the gases and particles in the air. Blue light is scattered more than the other colors because it travels as shorter, smaller waves. This is why we see a blue sky most of the time.
CB_GENERAL
EV_002neutral
Blue light waves are shorter than red light waves. Blue light is scattered in all directions by the tiny molecules of air in Earth's atmosphere. Blue is scattered more than other colors because it travels as shorter, smaller waves.
CB_GENERAL
EV_003neutral
Closer to the horizon, the sky fades to a lighter blue or white. The sunlight reaching us from low in the sky has passed through even more air than the sunlight reaching us from overhead. As the sunlight has passed through all this air, the air molecules have scattered and rescattered the blue light many times in many directions.
CB_GENERAL
EV_004neutral
The sky is blue due to a phenomenon called Raleigh scattering. This scattering refers to the scattering of electromagnetic radiation (of which light is a form) by particles of a much smaller wavelength. Sunlight is scattered by the particles of the atmosphere, and the smallest wavelengths of light tend to scatter easier. These shorter wavelengths correspond to blue hues, hence why when we look at the sky, we see it as blue.
CB_GENERAL
EV_005neutral
At sunset and sunrise, the angle at which sunlight enters the atmosphere is significantly changed, and most of the blue and green (shorter) wavelengths of light are scattered even before reaching the lower atmosphere, so we see more of the orange and red colours in the sky.
CB_GENERAL
EV_006neutral
Photos from NASA's rovers and landers on Mars have shown us that during the daytime, the Martian sky takes on an orange or reddish color. But as the Sun sets, the sky around the Sun begins to take on a blue-gray tone.
CB_GENERAL
EV_007neutral
I asked my science teacher and he said it was because the ozone layer is like a big mirror and the blue colours are the oceans on Earth.
CB_GENERAL
EV_008neutral
Sunlight reaches Earth's atmosphere and is scattered in all directions by all the gases and particles in the air. Blue light is scattered more than the other colors because it travels as shorter, smaller waves. This is why we see a blue sky most of the time.
CB_GENERAL
EV_009neutral
Blue light waves are shorter than red light waves. Blue light is scattered in all directions by the tiny molecules of air in Earth's atmosphere more than other colors because it travels as shorter, smaller waves.
CB_GENERAL
EV_010neutral
Closer to the horizon, the sky fades to a lighter blue or white because sunlight reaching from low in the sky has passed through even more air than sunlight reaching from overhead, causing air molecules to scatter and rescatter the blue light many times in many directions.
CB_GENERAL
EV_011neutral
During the daytime, the Martian sky takes on an orange or reddish color, while at sunset the sky around the Sun begins to take on a blue-gray tone, demonstrating that sky color depends on what is in the atmosphere.
CB_GENERAL
EV_012neutral
The sky is blue with a single cloud, as referenced in the title of Kuniko Tsurita's manga collection, acknowledging the blue color of the sky as an observable phenomenon.
CB_GENERAL
EV_013neutral
During the day, blue light gets scattered the most, while in the evening even more blue light gets scattered, causing the sky to turn red because lower frequencies become visible without blue overshadowing them.
CB_GENERAL
EV_014neutral
Blue light is scattered more than other colors because it travels as shorter, smaller waves, which is why we see a blue sky most of the time.
CB_GENERAL
EV_015neutral
Sunlight reaches Earth's atmosphere and is scattered in all directions by all the gases and particles in the air, with blue light being scattered in all directions by tiny molecules of air.
CB_GENERAL
EV_016neutral
Closer to the horizon, the sky fades to a lighter blue or white because sunlight reaching from low in the sky has passed through more air, causing blue light to be scattered and rescattered many times.
CB_GENERAL
EV_017neutral
Rayleigh scattering causes the blue color of the sky at large angles to the direction of solar rays.
CB_GENERAL
EV_018neutral
For light frequencies well below the resonance frequency of the scattering medium, the amount of scattering is inversely proportional to the fourth power of the wavelength, meaning blue color is scattered much more than red color as light propagates through air.
CB_GENERAL
EV_019neutral
Since blue light wavelengths scatter more, the diffuse sky seen in daytime is blue.
CB_GENERAL
EV_020neutral
In 1871, Lord Rayleigh published papers on the color and polarization of skylight that quantified the scattering effect in terms of particulates' volumes and refractive indices, establishing the basic scientific model for the color of the sky.
CB_GENERAL
EV_021neutral
Blue light gets scattered the most during the day, while in the evening even more blue light gets scattered, allowing red and yellow colors to become visible.
CB_GENERAL
EV_022neutral
Blue light is scattered more than other colors because it travels as shorter, smaller waves, which is why we see a blue sky most of the time.
CB_GENERAL
EV_023neutral
Sunlight reaches Earth's atmosphere and is scattered in all directions by all the gases and particles in the air, with blue light being scattered more than other colors, resulting in a blue sky.
CB_GENERAL
EV_024neutral
The sky's blue color depends on life on Earth and the makeup of our planet's ozone layer; without microbial life's impact on atmospheric composition, the clear daytime sky would probably lack its distinctive blue color.
CB_GENERAL
EV_025neutral
Closer to the horizon, the sky fades to a lighter blue or white because sunlight has passed through more air, causing blue light to be scattered and rescattered many times, mixing colors together.
CB_GENERAL
EV_026neutral
The book 'Why the Sky Is Blue' provides a historical and scientific journey showing various ways people in different times and places have explained why the sky looks blue, from ancient myths to cutting-edge science of optics and statistical physics.
CB_GENERAL
EV_027neutral
On Mars, the sky takes on an orange or reddish color during daytime, but at sunset the sky around the Sun takes on a blue-gray tone, demonstrating that sky color depends on atmospheric composition.
CB_GENERAL
EV_028neutral
Blue light is scattered more than other colors because it travels as shorter, smaller waves, which is why we see a blue sky most of the time.
CB_GENERAL
EV_029neutral
Sunlight reaches Earth's atmosphere and is scattered in all directions by all the gases and particles in the air, with blue light being scattered more than other colors.
CB_GENERAL
EV_030neutral
It is easy to see that the sky is blue, and this observation has been the subject of scientific inquiry for a long time.
CB_GENERAL
EV_031neutral
Blue light waves are shorter than red light waves, and blue light is scattered in all directions by the tiny molecules of air in Earth's atmosphere.
CB_GENERAL
EV_032neutral
Closer to the horizon, the sky fades to a lighter blue or white because sunlight has passed through more air, causing blue light to be scattered and rescattered many times.
CB_GENERAL
EV_033neutral
A Reddit user questions and seeks to understand why the sky is blue and changes colors, indicating that the blue color of the sky is a commonly observed phenomenon.
CB_GENERAL
EV_034neutral
The human eye can see the Milky Way in Bortle 1 or 2 zones (areas with minimal light pollution), suggesting the eye's visual perception capabilities in low-light astronomical conditions.
CB_GENERAL
EV_035neutral
The human eye can perceive and distinguish visual details (such as sunrise colors and brightness) that camera sensors struggle to capture with the same fidelity, indicating the eye's superior dynamic range and color perception capabilities.
CB_GENERAL
EV_1771422802698neutral
Rayleigh scattering results from the electric polarizability of particles, where the oscillating electric field of a light wave acts on charges within a particle, causing them to move at the same frequency and become a small radiating dipole
other
probative: high
CB_01
EV_1771422820284neutral
Shorter wavelengths are more energetic than longer ones; blue light has more energy than red light
other
probative: medium
CB_03
EV_1771422820285neutral
Gases and particles in Earth's atmosphere scatter sunlight in all directions
other
probative: medium
CB_03
EV_1771422851211neutral
Molecular scattering is usually called Rayleigh scattering, as it was first studied and explained by Lord Rayleigh, and is responsible for the blue sky phenomenon
other
probative: medium
CB_03
EV_1771422874790neutral
Blue light waves scatter at a rate about four times stronger than red light waves. The volume of scattering by the shorter blue light waves, along with additional scattering by violet and indigo, dominate scattering by the remaining color wavelengths.
government_report
probative: high
CB_05
EV_1771422874792neutral
The attenuation of a direct beam of sunlight by Rayleigh scattering is described by an equation with the cross-section for scattering being inversely proportional to wavelength raised to the fourth power (1/λ4). Rayleigh scattering explains the blue color of the sky on a clear day, since the shortest visible wavelengths, in the blue and violet, are scattered more efficiently than are longer wavelengths.
other
probative: high
CB_05
EV_1771422891613neutral
Single scattering is an appropriate approximation to modeling sky radiance in the vast majority of cases, but multiple scattering can contribute to sky radiance, particularly at larger distances from light sources.
peer_reviewed_study
probative: medium
CB_05
EV_1771422921511neutral
When the sunlight path length in the atmosphere is relatively short (since the zenith angle is very small) at noon time, nearly all of the violet and blue light are isotropically scattered and form the usual blue sky.
other
probative: medium
CB_05
EV_1771422999011neutral
Rayleigh scattering is implemented in the MODIS atmospheric correction algorithm to account for molecular scattering effects in the atmosphere, with scattering cross sections that vary with wavelength according to theoretical principles.
other
probative: medium
CB_10
EV_1771422999014neutral
Rayleigh scattering accounts for scattering, local field effects (Lorentz-Lorenz), and depolarization from non-sphericity of molecules/particles (King correction factor), with the interaction of light at wavelengths much larger than molecular size giving rise to Rayleigh scattering.
peer_reviewed_study
probative: medium
CB_01