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Stars distances

Wire sparklers are wires coated with pyrotechnic composition which are hand-held and produce a gende spray of gold sparks from iron filings. Fountains are cardboard tubes filled with chemical mixtures that produce a spray of color and sparks extending 2—5 m into the air. Roman candles are cylindrical tubes which repeatedly fire colored stars distances of 5—20 m into the air. These items typically contain 5—12 stars. [Pg.349]

Star Constellation Type of star Distance (light- years) Mass Radius Surface Intrinsic Magni-(solar (solar temperature brightness tude masses) radius) (Fahrenheit) (relative to sun) ... [Pg.321]

The accuracy of the radius and temperature determination will depend on the quality of the spectral fit (and thus on the sensitivity and resolution of the spectrum), the precision of the Sun-star distance, the cloud coverage and also the distribution of brightness temperatures over the planetary surface. Assuming the effective temperature of our planet was due exclusively from radiation to the surface instead of an atmosphere layer (the average equilibrium temperature of Earth is about 265 K instead of the 288 K surface temperature), would only introduce a few percent error on the derived Earth radius. [Pg.151]

Dendrites can grow at constant speed at arbitrarily small undercooling A, but usually a non-zero value of the anisotropy e is required. The growth pattern evolving from a nucleus acquires a star-shaped envelope surrounding a well-defined backbone. The distances between the corners of the envelope increase with time. For small undercooling we can use the scaling relation for the motion of the corners as for free dendrites [103-106] with tip... [Pg.891]

Table 7.1 shows the construction of a typical activity chart using one of many computer spreadsheet packages. The cross (-F) identifies an activity in the plant and stars ( ) in the vertical lines denote where access to other activities is needed or an interrelationship exists. A wide scattering of the stars away from the diagonal line of crosses indicates large distances between the activities and thus large communicating distances. [Pg.74]

A feature of PC spreadsheets is that the position of rows or columns can be changed at the touch of a key, so the sequence of the rows of activities can be rapidly altered, and the position of the columns varied to preserve the diagonal pattern of crosses. This exercise can be executed a number of times to reduce the scatter of the stars away from the diagonal line and reduce the communicating distances between the activities. This has been carried out, and the result is shown in Table 7.2, where it can be seen that the stars are clustered more closely around the diagonal line. The list now shows the activities arranged in a preferred order of sequence. [Pg.74]

Something else should be said about the impact of accommodation- When the (general) theory concerned is strongly supported independently of the fact at issue, the accommodation of some fact, even in this ad hoc way, may well still supply the best explanation that science can currently supply for that fact. So, for example, the best explanation in, say, 1700 for the observation of no stellar parallax was surely the Copemican one—that there must in fact be an apparent parallactic motion but that even the nearest stars are so far away as to make the effect too small to be detected by even the best available telescopes. (Here, as before with Ptolemy and with scientific creationism, we use the phenomenon—no observed parallax—to fix (in this case in a rather loose way) an otherwise free parameter in the theory (distance to the nearest star).)... [Pg.62]

The idea is to select light beams coming from the elongated LGS in such a way that taken individually, they have the same properties as if they were coming from an infinite distance, as seen by the wavefront sensor. The concept is called PIGS for Pseudo-Infinite Guide Stars and should be tested on-sky in 2003. [Pg.84]

The coherent propagation of star light through optical fibres over long distance has been mainly investigated at IRCOM and kilometric linkages are now possible. The two main points to be managed are ... [Pg.299]

Take a system of two gravitationally bounded stars. Tliis system being non-spherieally symmetric and non-static, looses potential energy via emission of gw. This in turn results in a decrease of the distance r between the two stars and and increase of the angular velocity u. With the following definitions ... [Pg.311]

The numbers that scientists use range from enormous to extremely tiny. The distances between the stars are literally astronomical—the star nearest to the sun is 23 500000000000 miles from it. As another example, the number of atoms of chlorine in 35.5 g of chlorine is 602000000000000000000000, or 602 thousand billion billion. The diameter of one chlorine atom is... [Pg.13]

Equation (31) applies to monodisperse systems. For polydisperse systems Rg reflects a high-order moment of the distribution, the ratio of the 8th to the 6th moment of the distribution in mean size. For this reason Rg will correlate with the largest sizes of a distribution. There are several advantages to Rg as a measure of size over the end-to-end distance. For branched, star and ring structures the end-to-end distance has no clear meaning while Rg retains its meaning. Further, Rg is directly measured in static scattering measurements so it maintains a direct link to experiment. [Pg.133]

Long-period comets their extended ellipsoidal orbits reach far outside our solar system (up to half the distance to the next fixed star). This group includes the comet Kohoutek, discovered in the 1970s, which requires about 75,000 years for a single orbit. [Pg.59]

The search for extrasolar life requires us to find planets outside the solar system. But since stars are only visible as small dots of light, it will be very difficult to find planets in outer space, since these do not emit light. This is true even for the nearest star, Alpha Centauri, which is about 4.3 light years away (roughly 7,000 times the distance from the sun to Pluto). [Pg.293]

The transit method requires that the central star, the planet and the observer are connected by a line of sight. The dark planet passes across the light source and thus diminishes its light intensity to some extent. Observation is only possible when observer, star and planet are in a favourable position, i.e., the planet lies between the star and the observer. In spite of this requirement, the method permits the discovery of planets of about the size of the Earth information is also available on the size, mass and density of the planet as well as on its orbit. Because of its limits of applicability, this method is not often used. In the case of the star OGLE-TR-56, it was possible to detect an extrasolar planet, the orbit of which is very close to its sun only a twentieth of the distance of Mercury away from it. The temperature of the planet was determined to be around 1,900 K its diameter is about 1.3 times larger than that of Jupiter, its density about 500 kg/m3 (Brown, 2003 Konacki, 2003). [Pg.294]

The fourth method, astronomical measurement, is (like the Doppler method) based on the observation and measurement of tiny motions of a star which are due to the mass(es) of the orbiting planet(s). A primary goal of the Space Interferometry Mission (SIM) is the discovery of planets similar to Earth, which orbit around stars like the sun. The SIM is due to start in 2009, and the measurements carried out will increase the accuracy of determinations of distances of stars in our galaxy several hundred times. Exact information can be found in the catalogue which forms part... [Pg.295]

The detection of small extrasolar planets (of around the size of the Earth) will be done by registering the infrared light which they emit. Interference filters will blot out the light emitted by the star in question. Because of the huge distance from the Earth, effects due to its atmosphere and its IR radiation will not interfere. Darwin is intended not only to discover planets but to analyse their atmospheres for possible signs of life. [Pg.296]

Unlike the field stars, the open clusters show enhanced values of [Na/Fe] ( 0.2) and [Al/Fe] ( 0.1). Sodium and aluminum seem to be high and show a large dispersion at all ages and Galactocentric distances. There is recent evidence that... [Pg.8]


See other pages where Stars distances is mentioned: [Pg.24]    [Pg.24]    [Pg.11]    [Pg.707]    [Pg.142]    [Pg.755]    [Pg.892]    [Pg.6]    [Pg.154]    [Pg.448]    [Pg.749]    [Pg.31]    [Pg.84]    [Pg.206]    [Pg.243]    [Pg.250]    [Pg.253]    [Pg.373]    [Pg.462]    [Pg.123]    [Pg.313]    [Pg.335]    [Pg.4]    [Pg.32]    [Pg.39]    [Pg.40]    [Pg.97]    [Pg.100]    [Pg.26]    [Pg.298]    [Pg.11]    [Pg.5]    [Pg.16]   
See also in sourсe #XX -- [ Pg.2 , Pg.3 , Pg.4 , Pg.5 , Pg.6 , Pg.7 , Pg.8 , Pg.9 , Pg.10 , Pg.11 , Pg.12 , Pg.13 , Pg.140 , Pg.206 ]




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