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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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Julian year<br />

Gregorian Date (midnight) Julian Date (UTC) Modified Julian Date (UTC)<br />

Jan 1, 1900 2415020.5 15020<br />

Jan 1, 1980 2444239.5 44239<br />

Jan 1, 2000 2451544.5 51544<br />

For more information, see:<br />

http://www.capecod.net/ pbaum/date/back.htm<br />

(<strong>and</strong> http://tycho.usno.navy.mil/systime.html)<br />

Julian year See year.<br />

Juliet Moon of Uranus also designated UXI.<br />

Discovered by Voyager 2 in 1986, it is a small,<br />

irregular body, approximately 42 km in radius.<br />

Its orbit has an eccentricity of 0.0005, an inclination<br />

of 0 ◦ , a precession of 223 ◦ y −1 , <strong>and</strong> a<br />

semimajor axis of 6.44 × 10 4 km. Its surface is<br />

very dark, with a geometric albedo of less than<br />

0.1. Its mass has not been measured. It orbits<br />

Uranus once every 0.493 Earth days.<br />

Junge particle distribution A power-law<br />

distribution function [particles m −3 µm −1 ] often<br />

used to describe the particle concentration<br />

[particles m −3 ] per unit size interval [µm] vs.<br />

equivalent spherical diameter of particles; the<br />

number density for particles of equivalent diameter<br />

x is proportional to x −k . In natural waters<br />

k is typically 3 to 5.<br />

Juno Third asteroid to be discovered, in<br />

1804. Dimensions 230 by 288 km. Orbit: semimajor<br />

axis 2.6679 AU, eccentricity 0.25848, inclination<br />

to the ecliptic 12 ◦ .96756, period 4.358<br />

years.<br />

Jupiter A gas giant, the fifth planet from<br />

the sun with orbital semimajor axis 5.20AU<br />

(778,330,000 km), orbital eccentricity 0.0483;<br />

its orbital period is 11.8623 years. Jupiter is the<br />

largest planet, with equatorial radius 71,492 km,<br />

<strong>and</strong> mass 1.9 × 10 27 kg; its mean density is<br />

1.33 gm/cm 3 . It has a surface rotational period<br />

of 9.841 hours. Jupiter has an orbital inclination<br />

of 1.308 ◦ <strong>and</strong> an axial tilt of 3.12 ◦ . Jupiter has<br />

an absolute magnitude of −2.7, making it usually<br />

the fourth brightest object in the sky, after<br />

the sun, moon, <strong>and</strong> Venus; occasionally Mars<br />

exceeds Jupiter in brightness.<br />

© 2001 by CRC Press LLC<br />

262<br />

The model structure of Jupiter envisions a<br />

rocky core of order 10 to 15 M⊕, at a temperature<br />

≈ 2×10 5 K, maintained by the gravitational<br />

compression of the planet. Because of this heating,<br />

Jupiter radiates considerably more energy<br />

than it receives from the sun. Above this core is<br />

a layer of liquid metallic hydrogen (at pressure<br />

depths exceeding 4 million atmospheres). Liquid<br />

metallic hydrogen is an electrical conductor<br />

<strong>and</strong> large scale currents in this material produce<br />

Jupiter’s magnetic field, via the dynamo effect.<br />

Jupiter’s field is 14 times stronger at Jupiter’s<br />

“surface” equator (4.3 Gauss), than is Earth’s at<br />

its equator (0.3 Gauss). Jupiter’s magnetic field<br />

is roughly dipolar, with its axis offset by 10,000<br />

km from the center of the planet <strong>and</strong> tipped 11 ◦<br />

degrees from Jupiter’s rotation axis. Jupiter’s<br />

magnetosphere extends more than 650 million<br />

kilometers outward, but only a few million kilometers<br />

sunward.<br />

Above the metallic hydrogen is a region composed<br />

primarily of ordinary molecular hydrogen<br />

(90%) <strong>and</strong> helium (10%) which is liquid in the<br />

interior <strong>and</strong> gaseous further out.<br />

Three distinct cloud layers exist in the atmosphere,<br />

consisting of ammonia ice, ammonium<br />

hydrosulfide, <strong>and</strong> a mixture of ice <strong>and</strong><br />

water. Jupiter’s atmosphere has high velocity<br />

winds (exceeding 600 km/h), confined in latitudinal<br />

b<strong>and</strong>s, with opposite directions in adjacent<br />

b<strong>and</strong>s. Slight chemical <strong>and</strong> temperature differences<br />

between these b<strong>and</strong>s are responsible for<br />

the colored b<strong>and</strong>s that dominate the planet’s appearance.<br />

The reddish colors seem to be associated<br />

with the highest clouds, the bluish colors<br />

with the deepest. Intermediate clouds have<br />

brown-cream-white colors.<br />

Jupiter posseses a very long-lived atmospheric<br />

phenomenon, the Great Red Spot, which<br />

has been observed for over 300 years. This is<br />

a reddish colored elliptical shaped storm, about<br />

12,000 by 25,000 km.<br />

Jupiter has three faint <strong>and</strong> small, low (about<br />

0.05) albedo rings (called Halo, Main, <strong>and</strong> Gos-

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