FACTOID # 76: The fourteen unhappiest countries are all in Eastern Europe.
 
 Home   Encyclopedia   Statistics   Countries A-Z   Flags   Maps   Education   Forum   FAQ   About 
 
 
 
WHAT'S NEW
RECENT ARTICLES
More Recent Articles »
 

SEARCH ALL

FACTS & STATISTICS    Advanced view

Search encyclopedia, statistics and forums:

 

 

(* = Graphable)

 

 


Encyclopedia > 203 Pompeja
203 Pompeja
Discovery A
Discoverer C. H. F. Peters
Discovery date September 25, 1879
Alternate
designations
A895 EA B
Category Main belt
Orbital elements C
Epoch 30 January 2005 (JD 2453400.5)
Eccentricity (e) 0.061
Semi-major axis (a) 409.322 Gm (2.736 AU)
Perihelion (q) 384.513 Gm (2.57 AU)
Aphelion (Q) 434.131 Gm (2.902 AU)
Orbital period (P) 1653.102 d (4.53 a)
Mean orbital speed 18.01 km/s
Inclination (i) 3.185°
Longitude of the
ascending node
(Ω)
348.019°
Argument of
perihelion
(ω)
59.83°
Mean anomaly (M) 210.675°
Physical characteristics
Dimensions 116.0 km
Mass unknown
Density unknown
Surface gravity unknown
Escape velocity unknown
Rotation period 46.60 h
Spectral class DCX:
Absolute magnitude 8.76
Albedo 0.041
Mean surface
temperature
unknown

203 Pompeja is a quite large Main belt asteroid. Christian Heinrich Friedrich Peters (September 19, 1813 – July 18, 1890) was an American astronomer, and one of the first to discover asteroids. ... September 25 is the 268th day of the year (269th in leap years). ... 1879 was a common year starting on Wednesday (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 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 diameter of about 4880 km). ... 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. ... 2005 is a common year starting on Saturday of the Gregorian calendar and is the current year. ... The Julian day or Julian day number (JDN) is the number of SI days that have elapsed since 12 noon Greenwich Mean Time (UT or TT) on Monday, January 1, 4713 BC in the proleptic Julian calendar 1. ... 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, is the basic unit of length in the International System of Units (SI: Système International dUnités). ... 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. ... A day is any of several different units of time. ... A Julian year is the length of an average year in the Julian calendar, 365. ... 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 (or 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. ... Density (symbol: ρ - Greek: rho) is a measure of mass per unit of volume. ... It has been suggested that Law of universal gravitation be merged into this article or section. ... 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 an orbit within a... In astronomy, a rotation period is the time an astronomical object takes to complete one revolution around its rotation axis. ... The hour was originally defined in Egypt as 1/24 of a day, based on their duo-decimal numbering system (which counted finger joints on each hand). ... An asteroid is a small, solid object in our Solar System, orbiting the Sun. ... 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. ... An asteroid is a small, solid object in our Solar System, orbiting the Sun. ...


It was discovered by C. H. F. Peters on September 25, 1879 in Clinton and named after Pompeii, the Roman town destroyed in volcanic eruption in 79 AD. Christian Heinrich Friedrich Peters (September 19, 1813 – July 18, 1890) was an American astronomer, and one of the first to discover asteroids. ... September 25 is the 268th day of the year (269th in leap years). ... 1879 was a common year starting on Wednesday (see link for calendar). ... Clinton may refer to a number of persons or places. ... Ruins in Pompeii The city of Pompeii, along with Herculaneum and many smaller places around the Bay of Naples, were Roman municipalities destroyed during an eruption of the volcano Mount Vesuvius in 79 CE. The eruption was described by Pliny the Younger (see below), whose uncle Pliny the Elder died... The Roman Empire is the term conventionally used to describe the Ancient Roman polity in the centuries following its reorganization under the leadership of Octavian (better known as Caesar Augustus). ... A volcano is a geological landform (usually a mountain) where magma (rock of the Earths interior made molten or liquid by extremely high temperatures along with a reduction in pressure and/or the introduction of water or other volatiles) erupts through the surface of the planet. ... AD79 Events June 23 - Titus succeeds his father Vespasian as Roman emperor. ...


References

  • The Asteroid Orbital Elements Database
  • Minor Planet Discovery Circumstances
  • Asteroid Lightcurve Parameters
  • Asteroid Albedo Compilation


... | Previous asteroid | 203 Pompeja | Next asteroid | ...


202 Chryseïs is a large, lightly coloured Main belt asteroid. ... 204 Kallisto is a fairly typical, altough sizeable Main belt asteroid. ...

The minor planets
Vulcanoids | Main belt | Groups and families | Near-Earth objects | Jupiter Trojans
Centaurs | Trans-Neptunians | Damocloids | Comets | Kuiper belt | 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:
 
Astron. Astrophys. 334, 729-735 (1998) (2546 words)
In the present paper, a determination of the mass of Ceres from its gravitational perturbations on the orbits of 9 asteroids, whose names are given in Table 1, is discussed.
In the case of (203) Pompeja, old observations published in Goffin (1991), and not included in the MPC tape, were added.
It can be seen, looking at the last column of Table 6, that the effects of these perturbations on the values found for the mass of Ceres, although not very strong in general, are often non negligible, especially in the case of (203) Pompeja, one of the better candidates for the determination of the mass.
Pedigree of Michiel Robert WATERLANDER MSc (10004 words)
Married on 11-06-1856 in Haren to Josina Pompeja QUINTUS, born circa 1834 in Groningen.
Henri Denis Francois, born on 22-09-1837 in Kollumerland, died on 06-07-1900 in Leeuwarden at the age of 62.
203 Baronesse Albertine du TOUR, born on 08-01-1751, died on 23-10-1806 at the age of 55, daughter of Gerrit Martijn du TOUR (see also 406) and Maria A. van BAERT van CRANENBROEK (see also 407).
  More results at FactBites »


 
 

COMMENTARY     


Share your thoughts, questions and commentary here
Your name
Your comments

Want to know more?
Search encyclopedia, statistics and forums:

 


Lesson Plans | Student Area | Student FAQ | Reviews | Press Releases |  Feeds | Contact
The Wikipedia article included on this page is licensed under the GFDL.
Images may be subject to relevant owners' copyright.
All other elements are (c) copyright NationMaster.com 2003-5. All Rights Reserved.
Usage implies agreement with terms, 1022, m