1054 Forsytia/fɔːrˈsɪtiə/ is a darkbackground asteroid, approximately 46 kilometers in diameter, from the outer regions of theasteroid belt. It was discovered on 20 November 1925, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany and assigned provisional designation1925 WD.[14] It is named after the flowering plantforsythia, and marks the beginning of a sequence of 28 thematically named asteroids by the discoverer.[3]
Forsytia is a non-family asteroid from the main belt'sbackground population.[5] It orbits the Sun in theouter asteroid belt at a distance of 2.5–3.3 AU once every 5.00 years (1,826 days;semi-major axis of 2.92 AU). Its orbit has aneccentricity of 0.14 and aninclination of 11° with respect to theecliptic.[1] The asteroid was first observed asA907 EA at Heidelberg in March 1907. The body'sobservation arc begins with its official discovery observation in November 1925.[14]
Due to his many discoveries,Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between(1009) and(1200). This list also contained a sequence of 28 asteroids, starting with this asteroid, that were all named after plants, in particularflowering plants(also see list of minor planets named after animals and plants).[3]
In March 2002, a rotationallightcurve ofForsytia was obtained from photometric observations by American amateur astronomerJohn Gross at his Sonoran Skies Observatory (G94) in Arizona. Lightcurve analysis gave a well-definedrotation period of 7.650 hours with a brightness amplitude of 0.23magnitude (U=3).[12]
According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Forsytia measures between 42.867 and 53.04 kilometers in diameter and its surface has analbedo between 0.035 and 0.0750.[6][7][8][9][10][11] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0592 and a diameter of 45.42 kilometers based on anabsolute magnitude of 10.4.[4]
^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.