<\/p>\n
+ All rings of Uranus show azimuthal brightness<\/strong> variations.\n<\/p>\n <\/p>\n + A strong lightness contrast between a mid-valued yellow paint and a surrounding bright white makes the yellow appear to be green or brown, while a strong brightness<\/strong> contrast between a rainbow and the surrounding sky makes the yellow in a rainbow appear to be a fainter yellow, or white.\n<\/p>\n <\/p>\n + Neptune cannot be seen with naked eye alone, since Neptune’s normal brightness<\/strong> are between Apparent magnitudemagnitudes +7.7 and +8.0, which can be out-shined by Jupiter’s Galilean moons, the Ceres, and the asteroids 4 Vesta, 2 Pallas, 7 Iris, 3 Juno and 6 Hebe.\n<\/p>\n <\/p>\n + The apparent magnitude of a celestial object is a number that measures its brightness<\/strong> as seen by an observer on Earth.\n<\/p>\n <\/p>\n + It had brightness<\/strong> of +8.1 visual magnitude.\n<\/p>\n + The galaxy is the new record holder for the brightest starburst galaxy in the very distant universe, its brightness<\/strong> being a measure of its extreme star-formation rate.\n<\/p>\n <\/p>\n + Hertzsprung-Russell diagrams are graphs that measure each star’s brightness<\/strong> against its temperature or color.\n<\/p>\n <\/p>\n + In astronomy, a light curve is a graph that shows the brightness<\/strong> of light from a celestial object or region, over a certain amount of time.\n<\/p>\n <\/p>\n + Each setting of the three dimmers will produce a different result, either in color or in brightness<\/strong> or both.\n<\/p>\n <\/p>\n + Rules suggested to describe optical illusions such as simultaneous brightness<\/strong> contrast illusion, such as Wallach’s ratio rule cannot explain White’s illusion.\n<\/p>\n <\/p>\n + The vertical axis of a Hertzsprung-Russell diagram shows the luminosity or brightness<\/strong> of the stars, as if they were all measured from the same distance.\n<\/p>\n <\/p>\n + The imprint only happens if the screen is used at maximum brightness<\/strong> for a long time.\n<\/p>\n <\/p>\n + Other discoveries include Purkinje images, reflections of objects from structures of the eye, and the Purkinje shift, the change in the brightness<\/strong> of red and blue colours as light intensity decreases gradually at dusk.\n<\/p>\n <\/p>\n + Although its size has not been directly measured, calculations based on its brightness<\/strong> give it a diameter of between 61km, if its albedoreflectivity is similar to Charon’s 35 percent, and about 167km, if it has a reflectivity of 4 percent like the darkest Kuiper belt objects.\n<\/p>\n <\/p>\n + He made several corrections to Ptolemy’s star-list and did his own brightness<\/strong> and magnitude estimates which often differed from those in Ptolemy’s work.\n<\/p>\n <\/p>\n + Think of a dimmable light switch: the knob itself selects ‘ON’, ‘OFF’, or somewhere in between, controlling the brightness<\/strong> of the light.\n<\/p>\n <\/p>\n + In astronomy, the brightness<\/strong> of an object is given in terms of its absolute magnitude.\n<\/p>\n <\/p>\n + Because of AMOLED\u2019s reduced maximum brightness<\/strong> and lack of backlighting, AMOLED displays may be difficult to view in direct sunlight compared to LCDs..\n<\/p>\n <\/p>\n + White’s illusion is a brightness<\/strong> illusion.\n<\/p>\n <\/p>\n + Objects of known brightness<\/strong> are called “standard candles”.\n<\/p>\n <\/p>\n + The brightness<\/strong> of Polaris can change.\n<\/p>\n <\/p>\n + The scattered light produces the brightness<\/strong> and color in clear skies.\n<\/p>\n <\/p>\n + Vega has served as the baseline for calibrating the astronomical brightness<\/strong> scale.\n<\/p>\n <\/p>\n + The star itself has an apparent brightness<\/strong> of 5.49, and because of this it is able to be seen from the Earth with binoculars, or with the naked eye if it is dark outside.\n<\/p>\n <\/p>\n + Since type Ia supernovae have a known brightness<\/strong> they can be used as standard candles to determine the distance to a galaxy once the stretch-factor is accounted for.\n<\/p>\n <\/p>\n + The ring is estimated to contribute 5% to the total brightness<\/strong> of Haumea.\n<\/p>\n <\/p>\n + The brightness<\/strong> of Neptune makes it hard to see the rings, which are much dimmer and the faintest rings still cannot be seen, even with vey powerful telescopes.\n<\/p>\n <\/p>\n + Courage, a very small and dim arc during the Voyager flyby, was seen to flare in brightness<\/strong> in 1998, while more recently it was back to its usual dimness but had advanced by an additional 8\u00b0 ahead of the other arcs.\n<\/p>\n <\/p>\n + Classical physics already had answers for the brightness<\/strong> of the bands of color that a hydrogen lamp produces, but the classical theory said that there should be a continuous rainbow, and not four separate color bands.\n<\/p>\n <\/p>\n + The Sun as seen from Mars is about as large as seen from Earth, and shines 40% of the light, approximately the brightness<\/strong> of a slightly cloudy afternoon on Earth.\n<\/p>\n <\/p>\n + The higher brightness<\/strong> of Europa would not overcome its greater distance from Jupiter, so it would not outshine Io.\n<\/p>\n <\/p>\n + These collections of stars by brightness<\/strong> and temperature are important when talking about stellar evolution.\n<\/p>\n <\/p>\n + An elliptical galaxy is a galaxy having an ellipsoidal shape, and a smooth, nearly featureless brightness<\/strong> profile.\n<\/p>\n <\/p>\n + The geometric albedo of an astronomical body is the ratio of its actual brightness<\/strong> at zero phase angle i.e.\n<\/p>\n <\/p>\n + Proxima Centauri increases its brightness<\/strong> randomly and magnetic force causes this.\n<\/p>\n <\/p>\n + Other metrics are absolute magnitude, which is an object’s intrinsic brightness<\/strong> at visible wavelengths, irrespective of distance.\n<\/p>\n <\/p>\n + Real-world examples include the loudness of a sound, the brightness<\/strong> of a star, or the Richter scale of earthquake intensity.\n<\/p>\n <\/p>\n + An astronomer could calculate the distance to this newly-discovered star by comparing its brightness<\/strong><\/strong> as seen from Earth against the brightness<\/strong><\/strong> for a certain color on the main sequence.\n<\/p>\n <\/p>\n + The size and brightness<\/strong> of a star determine where the circumstellar habitable zone is found around the star.\n<\/p>\n <\/p>\n + The brightness<\/strong> increases across the Electromagnetic spectrumspectrum, from X rays to radio waves.\n<\/p>\n <\/p>\n + Using this colour format, the brightness<\/strong> is stored apart from the colour.\n<\/p>\n <\/p>\n + This makes it sound louder and brighter so that it matches the brightness<\/strong> of the violin, especially as the violin is playing with normal tuning in the key of E flat, which sounds a soft key.\n<\/p>\n <\/p>\n + The least bright galaxies are one ten-billionth the brightness<\/strong> of what the human eye can see.\n<\/p>\n <\/p>\n + Cloud cover is indicated by the brightness<\/strong> of the map, while rain and snow are indicated by animated blue and white areas respectively.\n<\/p>\n <\/p>\n + If the player presses the L shoulder button, it can be used to adjust the backlit screen between five different brightness<\/strong> levels.\n<\/p>\n <\/p>\n + These lights were traditionally incandescent but are now increasingly light-emitting diodes with brightness<\/strong> control.\n<\/p>\n <\/p>\n + The display output devices convert the signal processing circuits’ brightness<\/strong> and colour information into the visible image displayed on a screen.\n<\/p>\n <\/p>\n + By the time Niels Bohr came out with his theory, most things about the light produced by a hydrogen lamp were known, but scientists still could not explain the brightness<\/strong> of each of the lines produced by glowing hydrogen.\n<\/p>\n <\/p>\n + Rather, Hertzsprung-Russell diagrams plot each star on a graph measuring the star’s brightness<\/strong> versus its temperature.\n<\/p>\n <\/p>\n + A main sequence star of a particular color has a narrow band of brightness<\/strong> when seen from a standard distance.\n<\/p>\n <\/p>\n + Most protostars show irregular brightness<\/strong> variations.\n<\/p>\n <\/p>\n + Werner Heisenberg took on the job of explaining the brightness<\/strong> or “intensity” of each line.\n<\/p>\n <\/p>\n + The reason for its brightness<\/strong> is not its intrinsic luminosity but its relative closeness to the Sun.\n<\/p>\n <\/p>\n + TV studios’ lightbulbs change brightness<\/strong> at twice the supply frequency.\n<\/p>\n <\/p>\n + White and White concluded that at a higher spatial frequency the grating of White’s illusion could be described by brightness<\/strong> assimilation.\n<\/p>\n <\/p>\n + Bohr’s theory provided a good explanation of many aspects of subatomic phenomena, but failed to answer why each of the colors of light produced by glowing hydrogen has a brightness<\/strong><\/strong> of its own, and the brightness<\/strong><\/strong> differences are always the same for each element.\n<\/p>\n <\/p>\n + Spectroscopy separates and measures the brightness<\/strong> of the different wavelengths.\n<\/p>\n <\/p>\n + Another easily observed effect is the drastic reduction in brightness<\/strong> of images of the sky and clouds reflected from horizontal surfaces.\n<\/p>\n <\/p>\n + The brightness<\/strong><\/strong> of the gray pieces appear to shift toward the brightness<\/strong><\/strong> of the top and bottom bordering stripes, that is, the gray bars with horizontal black regions on their top and bottom appear darker and those with white regions on their top and bottom appear lighter.\n<\/p>\n <\/p>\n + Even more dramatically, Libert\u00e9 appears to be fading away, being only 30% of its original 1989 brightness<\/strong> in 2003, and hardly visible in Hubble Space Telescope images from June 2005.\n<\/p>\n <\/p>\n + In botany, a light curve shows the photosynthetic response of a leaf or algae to the brightness<\/strong> of a light.\n<\/p>\n <\/p>\n + Neptune itself with a maximum brightness<\/strong> would be about that of the full moon on Earth.\n<\/p>\n <\/p>\n + Because the human eye is better at seeing brightness<\/strong> than seeing colour, we can apply a greater compression to the colour bytes.\n<\/p>\n <\/p>\n + In analyzing the varying distances, mulling through assumptions such as that they represented the brightness<\/strong> of the stars, he inadvertently found that they matched the distance of the stars from Earth on a scale of 1 meter =.799 light years within the margin of error for astronomical distances calculated today.West, John Anthony.\n<\/p>\n <\/p>\n + If there is more than one light source, there will be several shadows, with the overlapping parts darker, and various combinations of brightness<\/strong> or even colors.\n<\/p>\n <\/p>\n![\"brightness](\"https:\/\/englishteststore.net\/blog\/wp-content\/uploads\/2021\/09\/brightness-how-to-use-in-sentences.jpg\" "\\"brightness")
Example sentences of “brightness”:<\/h2>\n
+ The galaxy is the new record holder for the brightest starburst galaxy in the very distant universe, its brightness<\/strong> being a measure of its extreme star-formation rate.\r\n
+ Hertzsprung-Russell diagrams are graphs that measure each star's brightness<\/strong> against its temperature or color.\r\n
<\/pre>\nMore in-sentence examples of “brightness”:<\/h2>\n
+ Since type Ia supernovae have a known brightness<\/strong> they can be used as standard candles to determine the distance to a galaxy once the stretch-factor is accounted for.\r\n
+ The ring is estimated to contribute 5% to the total brightness<\/strong> of Haumea.\r\n
+ The brightness<\/strong> of Neptune makes it hard to see the rings, which are much dimmer and the faintest rings still cannot be seen, even with vey powerful telescopes.\r\n
<\/pre>\n