If the brightness is 'B' right now, when the object is at a distance 'D' from your eye, then
-- If the object moves closer, to only [ 1/2 D ] from you, the brightness increases to [ 4 B ].
-- If the object moves farther away, to [ 2 D ] from you, the brightnesses decreases to [ 1/4 B ].
A star who's brightness changes is called a variable star.Examples are:AlgolPolarisBetelgeuse.See related link for more information.
The apparent magnitude of Mercury varies because its brightness changes as it moves in its orbit about the sun. And the earth, from which we view Mercury and make a determination as regards it apparent magnitude, moves as well. It varies from -1.9 to 5.5 as we see it. (Some sources hold a -2.0 as a lower limit.) A link can be found below.
malay ko...
phases there are 8
By changes in the stars' brightness, and slight variations in their predicted location.
-- The size of the objects has no effect on the gravitational forces between them.The magnitude of the forces depends on the product of their masses, which arenot necessarily related to their size.-- The gravitational force between them decreases according to the square of thedistance between their centers. That means that if the distance doubles, the forcebecomes 1/4 as great, and if the distance multiplies by 5, the force becomes 1/25 as great.-- I don't understand what is meant by the "apparent magnitude of the objects".==========================Oh, wait! Don't go away. Are you talking about the apparent brightness of a staras its distance from us changes ? (There I go again ... changing an incomprehensiblequestion into one that makes sense, before I start laboring to answer my own question.)-- The apparent brightness of a light source acts according to the same "inverse square"law as the gravitational force does.-- Each "magnitude" of brightness of a sky object is actually a ratio of 2.1544 .(The 6th root of 100 . . . Don't ask!)-- So if I'm handling this correctly, that means that every time you move a starabout 1.4678 times farther from us, it appears less bright by 1 magnitude.
For nearby stars, the parallax method is used. Briefly, the star's apparent position changes, due to Earth's movement around the Sun. For objects that are farther away, several "standard candle" methods are used, meaning that the brightness of objects is measured that are assumed to have a more or less constant brightness; for example, "the brightest stars of a certain type of star, in a galaxy".
A star who's brightness changes is called a variable star.Examples are:AlgolPolarisBetelgeuse.See related link for more information.
There are many ways to calculate distance at huge scales. One popular way is using a Cepheid within the nebula. A Cepheid is a very luminous variable star (a star that changes brightness). The changing of brightness tells us a lot about the distance by measuring the period (time) and the luminosity. See the related link for more methods.
Hello
Several methods exist. A fairly obvious one is the parallax method - while Earth moves around the Sun, it changes its position by about 300 million km.; this will change the apparent position of nearby stars. For star clusters or galaxies that are further away, several "standard candle" methods exist, which basically consist of comparing the real luminosity of objects that have a known brightness (like certain types of stars) with their apparent luminosity.
The apparent magnitude of Mercury varies because its brightness changes as it moves in its orbit about the sun. And the earth, from which we view Mercury and make a determination as regards it apparent magnitude, moves as well. It varies from -1.9 to 5.5 as we see it. (Some sources hold a -2.0 as a lower limit.) A link can be found below.
A decrease in the star's temperature
Not calipers. Astronomers snap a photo, wait six months, then snap another. The apparent change in position with respect to much further background stars gives them a decent estimate, using the diameter of Earth's solar orbit as one leg of an extremely long isosceles triangle. We gauge distances to further stars using apparent brightness of Cepheid variables, and so on.
malay ko...
The diameter of the Moon doesn't change. The apparent (or angular) diameter changes a little, depending on the distance of the Moon from Earth, but this is not directly related to the phases of the Moon.
Distance between these two is 2960 miles. The distance changes according to the route taken. These change accordingly so these are approximate.