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Pole star

 
Medical Dictionary: daughter star

n.

One of the figures forming the diaster of a dividing cell. Also called polar star.

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A pole star is a visible star, especially a prominent one, that is approximately aligned with the Earth's axis of rotation; that is, a star whose apparent position is close to one of the celestial poles, and which lies (approximately) directly overhead when viewed from the Earth's North Pole or South Pole. There are potentially both northern and southern pole stars, but whether there is either depends on the current orientation of the Earth's axis, which moves over time (see precession of the equinoxes). The term the Pole Star usually refers to the star Polaris (colloquially referred to as the North Star), which is the current northern pole star.

Pole stars change over time because stars exhibit a slow continuous drift with respect to the Earth's axis. The primary reason for this is the precession of the Earth's rotational axis that causes its orientation to change over time. If the stars were fixed in space, precession would cause the celestial poles to trace out imaginary circles on the celestial sphere approximately once every 26,000 years, passing close to different stars at different times. However, the stars themselves exhibit motion relative to each other, and this so-called proper motion is another cause of the apparent drift of a pole star.

Pole stars are often used in celestial navigation. While other stars' positions change throughout the night, the pole stars' position in the sky essentially do not. Therefore, they are a dependable indicator of the direction toward the respective geographic pole, and their angle of elevation can also be used to determine latitude.

Contents

North pole

At the present time, Polaris is the pole star in the northern direction. Its mean position (taking account of precession and proper motion) will reach a maximum declination of +89°32'23", so 1657" or 0.4603° from the celestial north pole, in February 2102. (Its current declination is +89°15'50.8".) Its maximum apparent declination (taking account of nutation and aberration) will be +89°32'50.62", so 1629" or 0.4526° from the celestial north pole, on 24 March 2100.[1]

South pole

σ Octantis is the naked-eye star closest to the south celestial pole, but it is too faint to serve as a useful pole star. The Southern Cross constellation functions as an approximate southern pole constellation, by pointing to where a southern pole star would be. At the equator it is possible to see both Polaris and the Southern Cross.

Precession

Precession of Earth's axis around the ecliptical poles
Precession N.gif
North ecliptical pole
Precession S.png
South ecliptical pole

A consequence of the precession is a changing pole star. Currently Polaris is extremely well-suited to mark the position of the north celestial pole, as Polaris is a moderately bright star with a visual magnitude of 2.1 (variable), and it is located within a half degree of the pole.[2] On the other hand, Thuban in the constellation Draco, which was the pole star in 3000 BC, is much less conspicuous at magnitude 3.67 (one-fifth as bright as Polaris); today it is invisible in light-polluted urban skies.

The brilliant Vega in the constellation Lyra is often touted as the best north star (it fulfilled that role around 12000 BC and will do so again around the year AD 14000), however it never comes closer than 5° to the pole.

When Polaris becomes the north star again around 27800 AD, due to its proper motion it then will be farther away from the pole than it is now, while in 23600 BC it came closer to the pole.

It is more difficult to find the south celestial pole in the sky at this moment, as that area is a particularly bland portion of the sky, and the nominal south pole star is Sigma Octantis, which with magnitude 5.5 is barely visible to the naked eye even under ideal conditions. That will change from the eightieth to the ninetieth centuries, however, when the south celestial pole travels through the False Cross.

This situation also is seen on a star map. The orientation of the south pole is moving toward the Southern Cross constellation. For the last 2,000 years or so, the Southern Cross has nicely pointed to the south pole. By consequence, the constellation is no longer visible from subtropical northern latitudes, as it was in the time of the ancient Greeks.

Other planets

Pole stars of other planets are defined analogously: they are stars that most closely coincide with the projection of the planet's axis of rotation onto the celestial sphere. Different planets have different pole stars because their axes are oriented differently.

The location of the celestial poles of the planets is shown in the following table:

Planet North Celestial Pole South Celestial Pole
RA Dec RA Dec
Mercury 281.01 +61.45 101.01 −61.45
Venus 272.76 +67.16 92.76 −67.16
Earth +90.00 −90.00
Mars 317.68 +52.88 137.68 −52.88
Jupiter 268.05 +64.49 88.05 −64.49
Saturn 40.56 +83.54 220.56 −83.54
Uranus 257.43 −15.10 77.43 +15.10
Neptune 299.36 +43.46 119.36 −43.46
Pluto 313.02 +9.09 133.02 −9.09

The declination of Uranus' north celestial pole is negative as it spins 'backwards'. Pluto's north celestial pole would likewise be below the Earth's celestial equator were it not for the large angle of its orbit with respect to the ecliptic. Venus should have a negative declination also though the reference material omitted this.[5]

Some asteroids have more than one axis of rotation, possible due to impacts with other bodies. These asteroids tumble in space and have no pole stars. It is possible that a planet could be similarly affected, though unlikely as the much greater mass of a planet and its (usually) spherical shape make it much more unlikely for an impact to create a second axis of rotation.

In Bhagavata Purana

  • In Vedic Wisdom, the Pole star is called Dhruva, an ardent devotee of the god Vishnu, who was blessed to be in a high position in the sky.[citation needed]

According to Vishnu Puran; Dhruva [Pole Star] situated in the tail of a Porpoise shaped Galaxy and Center of our Universe. our Solar system is tied up with it by Aerial cords.

vishnu puran

THE form of the mighty Hari which is present in heaven, consisting of the constellations, is that of a porpoise, with Dhruva situated in the tail. As Dhruva revolves, it causes the moon, sun, and stars to turn round also; and the lunar asterisms follow in its circular path; for all the celestial luminaries are in fact bound to the polar-star by aerial cords. The porpoise-like figure of the celestial sphere is upheld by Náráyańa, who himself, in planetary radiance, is seated in its heart; whilst the son of Uttanápáda, Dhruva, in consequence of his adoration of the lord of the world, shines in the tail of the stellar porpoise . The upholder of the porpoise-shaped sphere is the sovereign of all, Janárddana. This sphere is the supporter of Dhruva; and by Dhruva the sun is upstayed. Upon the sun depends this world, with its gods, demons, and men. In what manner the world depends upon the sun, be attentive, and you shall hear.

References

  1. ^ Jean Meeus, Mathematical Astronomy Morsels Ch.50; Willmann-Bell 1997
  2. ^ "Precession of the Equinox". Astro 101. Western Washington University Planetarium. http://www.wwu.edu/depts/skywise/a101_precession.html. Retrieved July 3, 2009. 
  3. ^ 2004. Starry Night Pro, Version 5.8.4. Imaginova. ISBN 978-0-07-333666-4. www.starrynight.com
  4. ^ http://www.eknent.com/etc/mars_np.png
  5. ^ http://www.spaceflightweb.com/pfs/earth.html

Other resources

See also

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Medical Dictionary. The American Heritage® Stedman's Medical Dictionary Copyright © 2002, 2001, 1995 by Houghton Mifflin Company Read more
Wikipedia. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article "Pole star" Read more