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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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horse latitudes<br />

from the loci of the stars in an HR diagram,<br />

which is roughly horizontal, at least for some<br />

choicesoftemperatureindicator. RRLyraevariables,<br />

one of the common distance indicators,<br />

are horizontal branch stars. The corresponding<br />

phase for stars of higher metallicity is called<br />

the clump phase, while more massive stars pass<br />

through the phase without abrupt changes in<br />

their locations on the HR diagram. See clump<br />

star, CNO cycle, helium burning, HR diagram,<br />

metallicity.<br />

horse latitudes The latitudes approximately<br />

30 ◦ N <strong>and</strong> 30 ◦ S which are regions of calm winds<br />

<strong>and</strong> generally high pressure.<br />

horst An elevated block of crustal material<br />

forming a ridge or plateau, bounded by parallel<br />

normal or reverse faults. A horst is usually<br />

produced by compressional tectonic forces.<br />

hot dark matter See dark matter, hot.<br />

hot spot (1.) A bright, compact component<br />

observed in the radio lobes of powerful radio<br />

sources, such as radio galaxies <strong>and</strong> quasars.<br />

Hot spots are frequently found in radio source<br />

of Fanaroff–Riley class II, which includes the<br />

brightest lobe dominated radio source. Hot<br />

spots are ∼ 1 kpc in size, <strong>and</strong> they appear unresolved<br />

when observed at moderate resolution.<br />

Their radio spectrum is described by a powerlaw<br />

over the frequency <strong>and</strong> a spectral index<br />

≈−0.5, suggesting that radiation is emitted via<br />

a synchrotron process. Their location, often at<br />

the outer end of the jet, suggests that hot spots<br />

are the site of impact between the high speed<br />

particles of the jet <strong>and</strong> the lobes. See Fanaroff–<br />

Riley.<br />

(2.) In geophysics, areas of enhanced volcanic<br />

activity not directly associated with plate<br />

boundary volcanism, either ocean ridges or the<br />

volcanic lines behind subduction zones. Hot<br />

spots represent areas where magma from the<br />

mantle erupts directly onto the surface, creating<br />

features associated with fluid lavas such as<br />

flood basalts <strong>and</strong> shield volcanos. The Hawaiian<br />

isl<strong>and</strong>s show the passage of the Pacific Plate<br />

over a hot spot. Icel<strong>and</strong> is considered to be a hot<br />

spot because of its large volcanic flux. Hot spot<br />

volcanism is a common process on other plan-<br />

© 2001 by CRC Press LLC<br />

228<br />

ets, particularly Mars <strong>and</strong> Venus where many of<br />

the large volcanos are the result of this process.<br />

hot towers The cores of large cumulonimbus<br />

clouds in the intertropical convergence zone.<br />

See intertropical convergence zone.<br />

hour angle The angular distance on the celestial<br />

sphere measured westward along the celestial<br />

equator from the vernal equinox to the<br />

hour circle passing through the celestial object<br />

in question. It is equal to 360 ◦ minus the right<br />

ascension.<br />

HR (Hertzsprung–Russell) or color-magnitude<br />

diagram A plot of brightness or luminosity<br />

vs. some indicator of effective temperature<br />

for observed stars, calculated models of<br />

stars, or a comparison between the two. Such<br />

diagrams have been a primary tool for displaying<br />

<strong>and</strong> testing ideas of stellar structure <strong>and</strong> evolution<br />

since the early 20th century. Such a plot<br />

was first attempted for stars in the Pleiades in<br />

1910 by Hans Rosenberg, following advice from<br />

Karl Schwarzschild, while Einar Hertzsprung<br />

<strong>and</strong> Henry Norris Russell soon after considered<br />

stars of known distances in the solar neighborhood.<br />

The vertical axis can be luminosity in solar<br />

units or absolute magnitude or even apparent<br />

magnitude for a cluster of stars known to be<br />

all the same distance from us, either over a full<br />

range of wavelengths (bolometric luminosity) or<br />

over some restricted range of wavelengths (U, B,<br />

V ,R, I, etc., UBV colors). The horizontal axis<br />

can be effective temperature (especially in the<br />

case of models), a color index, or spectral type.<br />

Real stars do not populate such a diagram at<br />

r<strong>and</strong>om. Ninety percent (in a distance-limited<br />

sample) will fall on a diagonal from Hot-Bright<br />

(upper left) to Cool-Faint (lower right) called the<br />

main sequence. The scattering of stars above the<br />

main sequence are called red giants <strong>and</strong> supergiants;<br />

those fainter are sub-dwarfs <strong>and</strong> white<br />

dwarfs. A cluster of stars all with the same age<br />

<strong>and</strong> initial chemical composition has a characteristic<br />

HR diagram with signatures for age <strong>and</strong><br />

metallicity. An HR diagram representing observed<br />

stars normally shows individual symbols<br />

for each star.

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