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39 Laetitia (lə-tee'-shə (key)) is a large, bright main belt asteroid. In physics, an orbit is the path that an object makes, around another object, whilst under the influence of a source of centripetal force, such as gravity. ...
Image of the main asteroid belt between the orbits of Mars and Jupiter. ...
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. ...
A year is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ...
Inclination in general is the angle between a reference plane and another plane or axis of direction. ...
In astrodynamics, under standard assumptions any orbit must be of conic section shape. ...
Diameter is an AAA (authentication, authorization and accounting) protocol for applications such as network access or IP mobility. ...
A kilometre (American spelling: kilometer), symbol: km is a unit of length in the metric system equal to 1000 metres (from the Greek words Ïίλια (khilia) = thousand and μÎÏÏο (metro) = count/measure). ...
In astronomy, a rotation period is the time an astronomical object takes to complete one revolution around its rotation axis. ...
The hour (symbol: h) is a unit of time. ...
In astronomy one method of classifying stars is through the analysis of their absorption spectra, by this method stars are assigned a spectral class. ...
Approximately 17% of all known asteroids are of an S-type (for stony) composition. ...
In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standard luminosity distance away from us (in the absence of interstellar extinction!). It allows the overall brightnesses of objects to be compared without regard to distance. ...
Albedo is the measure of reflectivity of a surface or body. ...
Jean Chacornac (June 21, 1823 â September 23, 1873) was a French astronomer. ...
1856 was a leap year starting on Tuesday (see link for calendar). ...
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. ...
An asteroid is a small, solid object in our Solar System, orbiting the Sun. ...
It was discovered by J. Chacornac on February 8, 1856 and named after Laetitia, a minor Roman goddess of gaiety. Jean Chacornac (June 21, 1823 â September 23, 1873) was a French astronomer. ...
February 8 is the 39th day of the year in the Gregorian Calendar. ...
1856 was a leap year starting on Tuesday (see link for calendar). ...
Laetitia can mean several things: Laetitia was a minor Roman goddess of gaiety which make sense as Laetitia is the Latin word of happiness deriving from the root word laeta which means happy. ...
Roman mythology, the mythological beliefs of the people of Ancient Rome, can be considered as having two parts. ...
Aspects | Stationary, than retrograde | Opposition | Minimal distance (AU) | Maximum brightness (mag) | Stationary, than prograde | Conjunction to sun | | 07. June 2005 | 25. July 2005 | 1,59715 AE | 9,5 | 08. September 2005 | 25. March 2006 | | 17. October 2006 | 02. December 2006 | 1,64543 AE | 9,7 | 19. January 2007 | 25. July 2007 | | 12. January 2008 | 02. March 2008 | 2,05346 AE | 10,2 | 22. April 2008 | 13. October 2008 | | 03. April 2009 | 21.May 2009 | 1,93088 AE | 10,3 | 16. July 2009 | 10. January 2010 | | 04. August 2010 | 14. September 2010 | 1,46368 AE | 9,1 | 28. October 2010 | 17.May 2011 | | 22. November 2011 | 12. January 2012 | 1,84394 AE | 10,0 | 29. February 2012 | 27. August 2012 | | 13. February 2013 | 01. April 2013 | 2,08290 AE | 10,4 | 26.May 2013 | 14. November 2013 | | 12.May 2014 | 01. July 2014 | 1,72028 AE | 9,9 | 19. August 2014 | 25. February 2015 | | 25. September 2015 | 06. November 2015 | 1,54392 AE | 9,5 | 24. December 2015 | 02. July 2016 | | 25. December 2016 | 14. February 2017 | 1,99952 AE | 10,1 | 04. April 2017 | 27. September 2017 | | 16. March 2018 | 03.May 2018 | 2,01208 AE | 10,4 | 28. June 2018 | 20. December 2018 | | 03. July 2019 | 17. August 2019 | 1,51330 AE | 9,2 | 29. September 2019 | 18. April 2020 | | 02. November 2020 | 21. December 2020 | 1,73806 AE | 9,9 | 07. February 2021 | 09. August2021 |
photographic plate of 39 Laetitia in July 2005
Image taken with an advanced ccd … | Previous minor planet | 39 Laetitia | Next minor planet | … Image File history File links Download high resolution version (4048x3934, 3034 KB) Summary This is a scan of a photographic plate of the Asteroid 39 Laetitia. ...
Image File history File links Download high resolution version (4048x3934, 3034 KB) Summary This is a scan of a photographic plate of the Asteroid 39 Laetitia. ...
Image File history File links Laet1. ...
Image File history File links Laet1. ...
38 Leda is a large, dark main belt asteroid. ...
40 Harmonia is a large main belt asteroid. ...
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