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Encyclopedia > 1089 Tama
1089 Tama
Discovery A
Discoverer Okuro Oikawa
Discovery date November 17, 1927
Alternate
designations
A894 VA; A904 VD;
A919 HA; 1927 WB;
1930 ST; 1952 HE4 B
Category Main belt
Orbital elements C
Epoch November 26, 2005 (JD 2453700.5)
Eccentricity (e) 0.128
Semi-major axis (a) 331.131 Gm (2.213 AU)
Perihelion (q) 288.749 Gm (1.930 AU)
Aphelion (Q) 373.513 Gm (2.497 AU)
Orbital period (P) 1202.846 d (3.29 a)
Mean orbital speed 19.94 km/s
Inclination (i) 3.730°
Longitude of the
ascending node
(Ω)
71.565°
Argument of
perihelion
(ω)
354.336°
Mean anomaly (M) 236.255°
Physical characteristics D
Dimensions 12.9 km
Mass 2.2×1015? kg
Density 2.0? g/cm³
Surface gravity 0.0036? m/s²
Escape velocity 0.0068? km/s
Rotation period 0.6852±0.0002 d
Spectral class  ?
Absolute magnitude 11.6
Albedo 0.24
Mean surface
temperature
~179 K

1089 Tama is an asteroid orbiting the Sun. Okuro Oikawa (及川奥郎) was a Japanese astronomer. ... 17 November is also the name of a Marxist group in Greece. ... 1927 (MCMXXVII) was a common year starting on Saturday (link will take you to 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... The asteroid belt is a region of the solar system falling roughly between the planets Mars and Jupiter where the greatest concentration of asteroid orbits can be found. ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... November 26 is the 330th day (331st on leap years) of the year 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. ... Giga (symbol: G) is a prefix in the SI system of units denoting 109, or 1 000 000 000. ... The metre (Commonwealth English) or meter (American English) (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. ... In astronomy, a Julian year is a unit of time defined as exactly 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. ... Look up Second in Wiktionary, the free dictionary The second (symbol: s) is the SI base unit of time. ... 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, arc degree, or arcdegree), 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. ... For the majority of numbered asteroids, almost nothing is known apart from a few physical parameters. ... Mass is a property of physical objects that, roughly speaking, measures the amount of matter they contain. ... The international prototype, made of platinum-iridium, which is kept at the BIPM under conditions specified by the 1st CGPM in 1889. ... Density (symbol: ρ - Greek: rho) is a measure of mass per unit of volume. ... A cubic centimetre (cm3) is an SI derived unit of volume, equal to the volume of a cube with side length of 1 centi metre. ... Gravity is the force of attraction between massive particles. ... 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. ... 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. ... The kelvin (symbol: K) is the SI unit of temperature, and is one of the seven SI base units. ... An asteroid is a small, solid object in our Solar System, orbiting the Sun. ... The Sun (or Sol) is the star at the center of our Solar system. ...


A satellite, designated S/2003 (1089) 1, was identified based on lightcurve observations from 24 December 2003 to 5 January 2004 by Raoul Behrend, René Roy, Claudine Rinner, Pierre Antonini, Petr Pravec, Alan W. Harris, Stefano Sposetti, Russell I. Durkee, and Alain Klotz. This was announced on 12 January 2004. The moon, about 9 km in diameter, orbits 20 km away in 0.6852±0.0002 d (synchronously) and may actually be in contact with its primary. December 24 is the 358th day of the year in the Gregorian Calendar (359th in leap years). ... 2003 (MMIII) is a common year starting on Wednesday of the Gregorian calendar. ... January 5 is the 5th day of the year in the Gregorian calendar. ... 2004 (MMIV) was a leap year starting on Thursday of the Gregorian calendar. ... Pierre Antonini is a French astronomer. ... Petr Pravec is a Czech astronomer. ... Stefano Sposetti is a Swiss astronomer. ... January 12 is the 12th day of the year in the Gregorian calendar. ... 2004 (MMIV) was a leap year starting on Thursday of the Gregorian calendar. ...


External links

  • Discovery Circumstances: Numbered Minor Planets
  • Johnston Archive entry for 1089 Tama
  • IAUC 8265

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The minor planetsedit
Vulcanoids | Main belt | Groups and families | Near-Earth asteroids | 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:
 
1089 Tama at AllExperts (194 words)
1089 Tama is an asteroid orbiting the Sun.
A satellite, designated S/2003 (1089) 1, was identified based on lightcurve observations from 24 December 2003 to 5 January 2004 by Raoul Behrend, René Roy, Claudine Rinner, Pierre Antonini, Petr Pravec, Alan W. Harris, Stefano Sposetti, Russell I. Durkee, and Alain Klotz.
The moon, about 9 km in diameter, orbits 20 km away in 0.6852±0.0002 d (synchronously) and may actually be in contact with its primary.
  More results at FactBites »


 
 

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