542 Susanna
Encyclopedia
August Kopff
|-
| Discovery date
| August 15, 1904
|-
| Discovery site
| Heidelberg
|-
! bgcolor="#ffffcc" colspan="2" | Orbital elements
|-
| colspan="2" align="center" | Epoch
August 18, 2005 (JDCT
2453600.5)
|-
| Eccentricity (e)
| 0.142
|-
| Semimajor axis (a)
| 2.905 AU
|-
| Perihelion (q)
| 2.492 AU
|-
| Aphelion (Q)
| 3.317 AU
|-
| Orbital period
(P)
| 4.950 a
|-
| Inclination
(i)
| 12.076°
|-
| Longitude of the ascending node
(Ω)
| 153.279°
|-
| Argument of Perihelion (ω)
| 214.250°
|-
| Mean anomaly
(M)
| 124.220°
|}
August Kopff
August Kopff was a German astronomer who discovered several comets and asteroids. He worked in Heidelberg, then joined the Humboldt University of Berlin where he became the Director of the Institute for Astronomical Calculation.He discovered some comets, including periodic comet 22P/Kopff and the...
|-
| Discovery date
| August 15, 1904
|-
| Discovery site
| Heidelberg
Heidelberg
-Early history:Between 600,000 and 200,000 years ago, "Heidelberg Man" died at nearby Mauer. His jaw bone was discovered in 1907; with scientific dating, his remains were determined to be the earliest evidence of human life in Europe. In the 5th century BC, a Celtic fortress of refuge and place of...
|-
! bgcolor="#ffffcc" colspan="2" | Orbital elements
|-
| colspan="2" align="center" | Epoch
Epoch (astronomy)
In astronomy, an epoch is a moment in time used as a reference point for some time-varying astronomical quantity, such as celestial coordinates, or elliptical orbital elements of a celestial body, where these are subject to perturbations and vary with time...
August 18, 2005 (JDCT
Julian day
Julian day is used in the Julian date system of time measurement for scientific use by the astronomy community, presenting the interval of time in days and fractions of a day since January 1, 4713 BC Greenwich noon...
2453600.5)
|-
| Eccentricity (e)
| 0.142
|-
| Semimajor axis (a)
| 2.905 AU
Astronomical unit
An astronomical unit is a unit of length equal to about or approximately the mean Earth–Sun distance....
|-
| Perihelion (q)
| 2.492 AU
Astronomical unit
An astronomical unit is a unit of length equal to about or approximately the mean Earth–Sun distance....
|-
| Aphelion (Q)
| 3.317 AU
Astronomical unit
An astronomical unit is a unit of length equal to about or approximately the mean Earth–Sun distance....
|-
| Orbital period
Orbital period
The orbital period is the time taken for a given object to make one complete orbit about another object.When mentioned without further qualification in astronomy this refers to the sidereal period of an astronomical object, which is calculated with respect to the stars.There are several kinds of...
(P)
| 4.950 a
Julian year (astronomy)
In astronomy, a Julian year is a unit of measurement of time defined as exactly 365.25 days of 86 400 SI seconds each, totaling 31 557 600 seconds. The Julian year is the average length of the year in the Julian calendar used in Western societies in previous centuries, and for which the unit is...
|-
| Inclination
Inclination
Inclination in general is the angle between a reference plane and another plane or axis of direction.-Orbits:The inclination is one of the six orbital parameters describing the shape and orientation of a celestial orbit...
(i)
| 12.076°
|-
| Longitude of the ascending node
Longitude of the ascending node
The longitude of the ascending node is one of the orbital elements used to specify the orbit of an object in space. It is the angle from a reference direction, called the origin of longitude, to the direction of the ascending node, measured in a reference plane...
(Ω)
| 153.279°
|-
| Argument of Perihelion (ω)
| 214.250°
|-
| Mean anomaly
Mean anomaly
In celestial mechanics, the mean anomaly is a parameter relating position and time for a body moving in a Kepler orbit. It is based on the fact that equal areas are swept at the focus in equal intervals of time....
(M)
| 124.220°
|}
542 Susanna is a minor planet
Minor planet
An asteroid group or minor-planet group is a population of minor planets that have a share broadly similar orbits. Members are generally unrelated to each other, unlike in an asteroid family, which often results from the break-up of a single asteroid...
orbiting the Sun
Sun
The Sun is the star at the center of the Solar System. It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields...
.