residual elongation - ορισμός. Τι είναι το residual elongation
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Τι (ποιος) είναι residual elongation - ορισμός

IN ASTRONOMY, ANGULAR SEPARATION BETWEEN THE SUN AND A PLANET, WITH THE EARTH AS A REFERENCE POINT
Eastern elongation; Western elongation; Solar elongation; Greatest elongation
  • alt=An angle ε is drawn between two straight lines from Earth to the Sun, and from Earth to the planet. This is demonstrated for different positions along circular orbits, both for planets closer to the Sun (where the angle is always less than 90°), and for outer planets (for which the angle can range from 0° to 180°), while distinguishing east and west sides.

Residual-resistance ratio         
USUALLY DEFINED AS THE RATIO OF THE RESISTIVITY OF A MATERIAL AT ROOM TEMPERATURE AND AT 0 K
Residual resistance ratio; Residual–resistance ratio; Residual resistivity; Residual resitivity; Residual-resistivity ratio
Residual-resistivity ratio (also known as Residual-resistance ratio or just RRR) is usually defined as the ratio of the resistivity of a material at room temperature and at 0 K. Of course, 0 K can never be reached in practice so some estimation is usually made.
Residual income valuation         
ACCOUNTING TECHNIQUE
Residual Income Valuation
Residual income valuation (RIV; also, residual income model and residual income method, RIM) is an approach to equity valuation that formally accounts for the cost of equity capital. Here, "residual" means in excess of any opportunity costs measured relative to the book value of shareholders' equity; residual income (RI) is then the income generated by a firm after accounting for the true cost of capital.
Elongation (astronomy)         
In astronomy, a planet's elongation is the angular separation between the Sun and the planet, with Earth as the reference point. The greatest elongation of a given inferior planet occurs when this planet's position, in its orbital path around the Sun, is at tangent to the observer on Earth.

Βικιπαίδεια

Elongation (astronomy)

In astronomy, a planet's elongation is the angular separation between the Sun and the planet, with Earth as the reference point. The greatest elongation of a given inferior planet occurs when this planet's position, in its orbital path around the Sun, is at tangent to the observer on Earth. Since an inferior planet is well within the area of Earth's orbit around the Sun, observation of its elongation should not pose that much a challenge (compared to deep-sky objects, for example). When a planet is at its greatest elongation, it appears farthest from the Sun as viewed from Earth, so its apparition is also best at that point.

When an inferior planet is visible after sunset, it is near its greatest eastern elongation. When an inferior planet is visible before sunrise, it is near its greatest western elongation. The angle of the maximum elongation (east or west) for Mercury is between 18° and 28°, while that for Venus is between 45° and 47°. These values vary because the planetary orbits are elliptical rather than perfectly circular. Another factor contributing to this inconsistency is orbital inclination, in which each planet's orbital plane is slightly tilted relative to a reference plane, like the ecliptic and invariable planes.

Astronomical tables and websites, such as Heavens-Above, forecast when and where the planets reach their next maximum elongations.