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Axial Precession (Astronomy) - Miller, Frederic P. (Hrsg.) / Vandome, Agnes F. (Hrsg.) / McBrewster, John (Hrsg.)
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Miller, Frederic P. (Hrsg.) / Vandome, Agnes F. (Hrsg.) / McBrewster, John (Hrsg.):
Axial Precession (Astronomy) - Livres de poche

2009, ISBN: 9786130233112

[ED: Taschenbuch / Paperback], [PU: Alphascript Publishing], In astronomy, axial precession is a gravity-induced, slow and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers to the gradual shift in the orientation of Earth's axis of rotation, which, like a wobbling top, traces out a cone in a cycle of approximately 26,000 years (called a Great or Platonic year in astrology). The term "precession" typically refers only to this largest secular motion other changes in the alignment of Earth's axis nutation and polar motion are much smaller in magnitude. Earth's precession was historically called precession of the equinoxes because the equinoxes moved westward along the ecliptic relative to the fixed stars, opposite to the motion of the Sun along the ecliptic. This term is still used in non-technical discussions, that is, when detailed mathematics are absent. Historically, Hipparchus is credited with discovering precession of the equinoxes. The exact dates of his life are not known, but astronomical observations attributed to him by Ptolemy date from 147 BC to 127 BC., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 212, Selbstabholung und Barzahlung, PayPal, offene Rechnung, Banküberweisung, Interntationaler Versand

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Axial Precession (Astronomy) - Frederic P. Miller
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Frederic P. Miller:
Axial Precession (Astronomy) - Livres de poche

ISBN: 9786130233112

[ED: Taschenbuch], [PU: Alphascript Publishing], Neuware - In astronomy, axial precession is a gravity-induced, slow and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers to the gradual shift in the orientation of Earth's axis of rotation, which, like a wobbling top, traces out a cone in a cycle of approximately 26,000 years (called a Great or Platonic year in astrology). The term 'precession' typically refers only to this largest secular motion other changes in the alignment of Earth's axis nutation and polar motion are much smaller in magnitude. Earth's precession was historically called precession of the equinoxes because the equinoxes moved westward along the ecliptic relative to the fixed stars, opposite to the motion of the Sun along the ecliptic. This term is still used in non-technical discussions, that is, when detailed mathematics are absent. Historically, Hipparchus is credited with discovering precession of the equinoxes. The exact dates of his life are not known, but astronomical observations attributed to him by Ptolemy date from 147 BC to 127 BC., [SC: 0.00], Neuware, gewerbliches Angebot, 220x150x13 mm, [GW: 332g]

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Axial Precession (Astronomy) - Frederic P. Miller
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Frederic P. Miller:
Axial Precession (Astronomy) - nouveau livre

ISBN: 9786130233112

ID: 2804ac001bbd8e170bc767659a6a8895

In astronomy, axial precession is a gravity-induced, slow and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers to the gradual shift in the orientation of Earth's axis of rotation, which, like a wobbling top, traces out a cone in a cycle of approximately 26,000 years (called a Great or Platonic year in astrology). The term "precession" typically refers only to this largest secular motion other changes in the alignment of Earth's axis nutation and polar motion are much smaller in magnitude. Earth's precession was historically called precession of the equinoxes because the equinoxes moved westward along the ecliptic relative to the fixed stars, opposite to the motion of the Sun along the ecliptic. This term is still used in non-technical discussions, that is, when detailed mathematics are absent. Historically, Hipparchus is credited with discovering precession of the equinoxes. The exact dates of his life are not known, but astronomical observations attributed to him by Ptolemy date from 147 BC to 127 BC. Bücher / Naturwissenschaften, Medizin, Informatik & Technik / Physik & Astronomie

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Axial Precession (Astronomy) - Frederic P. Miller
Livre non disponible
(*)
Frederic P. Miller:
Axial Precession (Astronomy) - nouveau livre

ISBN: 9786130233112

ID: 2804ac001bbd8e170bc767659a6a8895

In astronomy, axial precession is a gravity-induced, slow and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers to the gradual shift in the orientation of Earth's axis of rotation, which, like a wobbling top, traces out a cone in a cycle of approximately 26,000 years (called a Great or Platonic year in astrology). The term "precession" typically refers only to this largest secular motion; other changes in the alignment of Earth's axis nutation and polar motion are much smaller in magnitude. Earth's precession was historically called precession of the equinoxes because the equinoxes moved westward along the ecliptic relative to the fixed stars, opposite to the motion of the Sun along the ecliptic. This term is still used in non-technical discussions, that is, when detailed mathematics are absent. Historically, Hipparchus is credited with discovering precession of the equinoxes. The exact dates of his life are not known, but astronomical observations attributed to him by Ptolemy date from 147 BC to 127 BC. Bücher / Naturwissenschaften, Medizin, Informatik & Technik / Physik & Astronomie

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Axial Precession (Astronomy)
Livre non disponible
(*)
Axial Precession (Astronomy) - Livres de poche

2009, ISBN: 9786130233112

[ED: Taschenbuch / Paperback], [PU: Alphascript Publishing], In astronomy, axial precession is a gravity-induced, slow and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers to the gradual shift in the orientation of Earth's axis of rotation, which, like a wobbling top, traces out a cone in a cycle of approximately 26,000 years (called a Great or Platonic year in astrology). The term "precession" typically refers only to this largest secular motion other changes in the alignment of Earth's axis nutation and polar motion are much smaller in magnitude. Earth's precession was historically called precession of the equinoxes because the equinoxes moved westward along the ecliptic relative to the fixed stars, opposite to the motion of the Sun along the ecliptic. This term is still used in non-technical discussions, that is, when detailed mathematics are absent. Historically, Hipparchus is credited with discovering precession of the equinoxes. The exact dates of his life are not known, but astronomical observations attributed to him by Ptolemy date from 147 BC to 127 BC., [SC: 0.00], Neuware, gewerbliches Angebot

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Détails sur le livre
Axial Precession (Astronomy): Astronomy, Earth, Cone (geometry), Great Year, Astrology, Secular phenomena, Nutation, Polar motion, Equinox, Ecliptic, Fixed stars, Sun, Hipparchus

In astronomy, axial precession is a gravity-induced, slow and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers to the gradual shift in the orientation of Earth's axis of rotation, which, like a wobbling top, traces out a cone in a cycle of approximately 26,000 years (called a Great or Platonic year in astrology). The term 'precession' typically refers only to this largest secular motion; other changes in the alignment of Earth's axis nutation and polar motion are much smaller in magnitude. Earth's precession was historically called precession of the equinoxes because the equinoxes moved westward along the ecliptic relative to the fixed stars, opposite to the motion of the Sun along the ecliptic. This term is still used in non-technical discussions, that is, when detailed mathematics are absent. Historically, Hipparchus is credited with discovering precession of the equinoxes. The exact dates of his life are not known, but astronomical observations attributed to him by Ptolemy date from 147 BC to 127 BC.

Informations détaillées sur le livre - Axial Precession (Astronomy): Astronomy, Earth, Cone (geometry), Great Year, Astrology, Secular phenomena, Nutation, Polar motion, Equinox, Ecliptic, Fixed stars, Sun, Hipparchus


EAN (ISBN-13): 9786130233112
ISBN (ISBN-10): 6130233116
Version reliée
Livre de poche
Date de parution: 2009
Editeur: Alphascript Publishing
212 Pages
Poids: 0,332 kg
Langue: eng/Englisch

Livre dans la base de données depuis 20.06.2009 23:12:55
Livre trouvé récemment le 18.09.2017 15:02:42
ISBN/EAN: 6130233116

ISBN - Autres types d'écriture:
613-0-23311-6, 978-613-0-23311-2


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