Skip to main content

  | मौसम…

411 समाचार
Public archive edition · Attributed source reporting with original dates · AI drafts are excluded

411 REFERENCE · Wikipedia

151 Abundantia

Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.

Main-belt asteroid September 2018 yes 151 Abundantia #D6D6D6 151 Abundantia.png Lightcurve based 3D model of 151 Abundantia Harvard, Numbured MPs J. Palisa Austrian Naval Obs. 1 November 1875 (151) Abundantia Main belt Abundantia æ b ə n ˈ d æ n ʃ i ə A875 VA; 1974 QS 2, 1974 QZ 2 http://ftp.lowell.edu/pub/elgb/astorb.html astorb The Asteroid Orbital Elements Database Lowell Observatory https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=151;cad=1 151 Abundantia JPL Small-Body Database NASA/Jet Propulsion Laboratory 12 May 2016 31 July 2016 (JD 2457600.5) 131.24 yr (47936 d) 0 2.6792 AU Gm on on 2.5049 AU Gm on 2.5921 AU Gm on 0.033623 4.17 yr (1524.3 d) 6.4348° 38.872° 141.90° 0.23617 ms / day 130.92° 45.37 0.9 km 9.864 h d on on 0.1728 0.0070.173DSN IRAS https://web.archive.org/web/20050224095554/http://dorothy.as.arizona.edu/DSN/IRAS/index_iras.html 2005-02-24 SLCSUMPUB 9.1 151 Abundantia is a stony main belt asteroid. It was discovered by Johann Palisa on 1 November 1875, from the Austrian Naval Observatory in Pula. The name was chosen by Edmund Weiss of the Vienna Observatory; although the name refers to Abundantia, a Roman goddess of luck, it was also chosen to celebrate the increasing numbers of asteroids that were being discovered in the 1870s.Schmadel Lutz D. Dictionary of Minor Planet Names https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA29 2003 Springer Science & Business Media 978-3-540-00238-3 29 Information from A. Harris as of 1 March 2001 indicates that 151 Abundantia is an S class (stony) asteroid with a diameter of 45.37 km and H = 9.24 .1728 and albedo of 0.03. The light curve collected over 6 nights from 2/16/2002 to 3/10/2002 confirmed the rotational period to be 19.718h.August 2022 Data from 2001 shows a diameter of 45.37 km.151 Abundantia http://btboar.tripod.com/lightcurves/id31.html https://web.archive.org/web/20110525140833/http://btboar.tripod.com/lightcurves/id31.html 2011-05-25 live 2009-03-11 An occultation by the asteroid was observed on 10 December 2017, showing the asteroid to be highly elongated, with dimensions of roughly 24 x 52 km.August 2022 References External links Lightcurve Data for 51 Abundantia https://web.archive.org/web/20110525140833/http://btboar.tripod.com/lightcurves/id31.html 25 May 2011 , Sunflower Observatory (739) Lightcurve plot of 151 Abundantia, Palmer Divide Observatory, B. D. Warner (2006) Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 ) Dictionary of Minor Planet Names, Google books Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center 151 150 Nuwa 151 152 Atala 000151 Category:Discoveries by Johann Palisa Category:Named minor planets 000151 000151 18751101