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Encyclopedia > 828 Lindemannia

828 Lindemannia

Name
Name Lindemannia
Designation 1916 ZX
Discovery
Discoverer J. Palisa
Discovery date August 29, 1916
Discovery site Vienna
Orbital elements
Epoch August 18, 2005 (JDCT 2453600.5)
Eccentricity (e) 0.036
Semimajor axis (a) 3.194 AU
Perihelion (q) 3.080 AU
Aphelion (Q) 3.308 AU
Orbital period (P) 5.708 a
Inclination (i) 1.135°
Longitude of the ascending node (Ω) 2.061°
Argument of Perihelion (ω) 286.488°
Mean anomaly (M) 288.197°

828 Lindemannia is a minor planet orbiting Sun. Johann Palisa (December 6, 1848 – May 2, 1925) was an Austrian astronomer, born in Opava, Czech Republic (then part of the Austrian Empire). ... August 29 is the 241st day of the year in the Gregorian Calendar (242nd in leap years), with 124 days remaining. ... 1916 (MCMXVI) is a leap year starting on Saturday (link will take you to calendar) // Events January-February January 1 -The first successful blood transfusion using blood that had been stored and cooled. ... Vienna (German: Wien [viːn]; Hungarian: Bécs, Czech: Vídeň, Slovak: Viedeň, Romany Vidnya; Serbian: Beč) is the capital of Austria, and also one of Austrias nine states (Land Wien). ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... August 18 is the 230th day of the year (231st in leap years) in the Gregorian calendar. ... 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. ... 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. ... 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. ... The astronomical unit (AU or au or a. ... The orbital period is the time it takes a planet (or another object) to make one full orbit. ... In astronomy, a Julian year is a unit of time defined as exactly 365. ... 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. ... 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. ... 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... The Sun (or Sol) is the star at the center of our Solar system. ...


External links

  • Discovery Circumstances: Numbered Minor Planets

… | Previous asteroid | 828 Lindemannia | Next asteroid | … 827 Wolfiana 827 Wolfiana is a minor planet orbiting Sun. ...



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:
 
Binoculars Asteroidal Occultations, 2002 Oct. 16, Nov. 3 & 10 (1477 words)
Occultation of pi Arietis by (828) Lindemannia, 2002 Nov. 10
The accuracy of the new path location is +/- 0.82 path-widths = 82 km, which means that even observers at the updated central line are not guaranteed an occultation, although there is a good chance of one occurring there.
The path for last weekend's Nephele occultation shifted almost a full path-width north, and that asteroid was twice the angular size of Lindemannia.
Asteroid_News.htm (0 words)
The effort to observe the occultation of a m = 5.4 star by the asteroid 828 Lindemannia over south Texas was organized by Paul Maley of the NASA Johnson Space Center Astronomical Society in Houston, Texas.
Observer #12, Becky Ramatowski was less than 2 km from the south limit of the asteroid and had a miss.
828 Lindemannia was discovered on August 29, 1916 by J. Palisa, in Vienna, Austria.
  More results at FactBites »


 
 

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