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Encyclopedia > 363 Padua
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363 Padua
Discovery A
Discoverer Auguste Charlois
Discovery date March 17, 1893
Alternate
designations
1893 S B
Category Main belt (Lydia)
Orbital elements C
Epoch 30 January 2005 (JD 2453400.5)
Eccentricity (e) 0.073
Semi-major axis (a) 410.982 Gm (2.747 AU)
Perihelion (q) 380.897 Gm (2.546 AU)
Aphelion (Q) 441.068 Gm (2.948 AU)
Orbital period (P) 1663.172 d (4.55 a)
Mean orbital speed 17.97 km/s
Inclination (i) 5.951°
Longitude of the
ascending node
(Ω)
64.995°
Argument of
perihelion
(ω)
294.64°
Mean anomaly (M) 5.679°
Physical characteristics
Dimensions 35 - 75 km
Mass unknown
Density unknown
Surface gravity unknown
Escape velocity unknown
Rotation period unknown
Spectral class unknown
Absolute magnitude 9.01
Albedo unknown
Mean surface
temperature
unknown

363 Padua is probably a typical Main belt asteroid. Auguste Honoré Charlois (November 26, 1864 – March 26, 1910) was a French astronomer who discovered 99 asteroids while working in Nice. ... Jump to: navigation, search March 17 is the 76th day of the year in the Gregorian Calendar (77th in Leap years). ... Jump to: navigation, search 1893 was a common year starting on Sunday (see link for calendar). ... The provisional designation of comets and asteroids are similar to each other: they both follow a pattern set in 1925 by the Minor Planet Center of the IAU. Historical designations At first, astronomers strove to assign symbols to the minor planets: 1 Ceres a stylized sickle 2 Pallas a lozenge... Minor planets, or planetoids are minor bodies of the Solar system orbiting the Sun (or of other planetary systems orbiting other stars) that are larger than meteoroids (the largest of which might be taken to be around 10 meters or so across) but smaller than major planets (Mercury having a... Image of the main asteroid belt between the orbits of Mars and Jupiter. ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... January 30 is the 30th day of the year in the Gregorian Calendar. ... Jump to: navigation, search 2005(MMV) is a common year starting on Saturday of the Gregorian calendar. ... The Julian day or Julian day number (JDN) is the number of days that have elapsed since 12 noon Greenwich Mean Time (UT or TT) on Monday, January 1, 4713 BC in the proleptic Julian calendar . ... In astrodynamics, under standard assumptions any orbit must be of conic section shape. ... In geometry, the semi-major axis (also semimajor axis) a applies to ellipses and hyperbolas. ... Giga (symbol: G) is a prefix in the SI system of units denoting 109, or 1 000 000 000. ... The metre, or meter (symbol: m) is the SI base unit of length. ... The astronomical unit (AU or au or a. ... This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ... This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ... The orbital period is the time it takes a planet (or another object) to make one full orbit. ... See also Day (language) A day (symbol: d) is a unit of time. ... A Julian year is the length of an average year in the Julian calendar, 365. ... Jump to: navigation, search The orbital speed of a body, generally a planet, a natural satellite, an artificial satellite, or a multiple star, is the speed at which it orbits around the barycenter of a system, usually around a more massive body. ... The second (symbol s) is a unit for time, and one of seven SI base units. ... Inclination is one of the six orbital parameters describing the shape and orientation of a celestial orbit and is the angular distance of the orbital plane from the plane of the reference (usually planets equator or the ecliptic), stated in degrees. ... A degree (in full, a degree of arc), usually symbolized °, is a measurement of plane angle, representing 1/360 of a full rotation. ... The Longitude of the ascending node () is one of the orbital elements used to specify the orbit of an object in space. ... The argument of the perihelion is one of the orbital elements describing the orbit of a planet. ... In the study of orbital dynamics the mean anomaly is a measure of time, specific to the orbiting body p, which is a multiple of 2π radians at and only at periapsis. ... Mass is a property of physical objects that, roughly speaking, measures the amount of matter they contain. ... Jump to: navigation, search Density (symbol: ρ - Greek: rho) is a measure of mass per unit of volume. ... Jump to: navigation, search It has been suggested that Law of universal gravitation be merged into this article or section. ... Jump to: navigation, search In physics, for a given gravitational field and a given position, the escape velocity is the minimum speed an object without propulsion, at that position, needs to have to move away indefinitely from the source of the field, as opposed to falling back or staying in... In astronomy, a rotation period is the time an astronomical object takes to complete one revolution around its rotation axis. ... Asteroids are assigned a type based on spectral shape, color, and sometimes albedo. ... In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standardized distance away. ... The albedo is a measure of reflectivity of a surface or body. ... Temperature is the physical property of a system which underlies the common notions of hot and cold; the material with the higher temperature is said to be hotter. ... Image of the main asteroid belt between the orbits of Mars and Jupiter. ... Jump to: navigation, search An asteroid is a small, solid object in our Solar System, orbiting the Sun. ...


It was discovered by Auguste Charlois on March 17, 1893 in Nice. Auguste Honoré Charlois (November 26, 1864 – March 26, 1910) was a French astronomer who discovered 99 asteroids while working in Nice. ... Jump to: navigation, search March 17 is the 76th day of the year in the Gregorian Calendar (77th in Leap years). ... Jump to: navigation, search 1893 was a common year starting on Sunday (see link for calendar). ... City motto: Nicæa civitas. ...



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Jump to: navigation, search 362 Havnia is a typical Main belt asteroid. ...

The minor planetsedit
Vulcanoids | Main belt | Groups and families | Near-Earth objects | Jupiter Trojans
Centaurs | Damocloids | Comets | Trans-Neptunians |Kuiper belt | Scattered disc | Oort cloud
For other objects and regions, see: Binary asteroids, Asteroid moons and the Solar system
For a complete listing, see: List of asteroids. For pronunciation, see: Pronunciation of asteroid names.

  Results from FactBites:
 
Northern Italy, Venice, Padua, Lake Orta, (2455 words)
The most splendid of its churches is "il Santo", that is, the basilica of St. Anthony of Padua.
On the high alter is a crucifix in bronze by Donatello, while the paintings in this church are by Mantegna, Paolo Veronese, and Tiepolo, with frescoes by Giotto and Altichiero.
Padua (Patavium) was the chief city of the Veneti, and boasts well of one of the world’s oldest Universities.
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