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1099 figneria, provisional designation 1928 rq, is an asteroid from the background population of the outer regions of the asteroid belt, approximately 26 kilometers in diameter.discovered by grigory neujmin at simeiz observatory in 1928, the asteroid was later named after russian revolutionary activist vera figner.on the same night, it was independently discovered by german astronomer max wolf at the heidelberg observatory in southwest germany.the minor planet center, however, only acknowledges the first discoverer.in october 1927, the asteroid was first identified as a917 uf at simeiz, where the body's observation arc begins 11 months later with its official discovery observation.it orbits the sun in the outer main belt at a distance of 2.3–4.1 au once every 5 years and 8 months (2,071 days).its orbit has an eccentricity of 0.28 and an inclination of 12° with respect to the ecliptic.the asteroid is also an assumed carbonaceous c-type asteroid.lightcurve analysis gave a rotation period of 13.577 hours with a brightness variation of 0.16 magnitude (u=3-).in january 2014, photometric observations at the palomar transient factory in california gave a period of 13.583 hours and an amplitude of 0.15 magnitude (u=2).the official naming citation was published in the planetenzirkular des astronomischen rechen-institut (ri 789).

1099 figneria | epoch | 2006-12-31 <tsp> 1099 figneria | orbitalperiod | 1799420000 <tsp> 1099 figneria | periapsis | 3492060000000 <tsp> 1099 figneria | apoapsis | 6057180000 kilometres

1099 Figneria, provisional designation 1928 RQ, is an asteroid from the background population of the outer regions of the asteroid belt, approximately 26 kilometers in diameter.

1099 figneria, provisional designation 1928 rq, is an asteroid from the background population of the outer regions of the asteroid belt, approximately 26 kilometers in diameter.discovered by grigory neujmin at simeiz observatory in 1928, the asteroid was later named after russian revolutionary activist vera figner.on the same night, it was independently discovered by german astronomer max wolf at the heidelberg observatory in southwest germany.the minor planet center, however, only acknowledges the first discoverer.in october 1927, the asteroid was first identified as a917 uf at simeiz, where the body's observation arc begins 11 months later with its official discovery observation.it orbits the sun in the outer main belt at a distance of 2.3–4.1 au once every 5 years and 8 months (2,071 days).its orbit has an eccentricity of 0.28 and an inclination of 12° with respect to the ecliptic.the asteroid is also an assumed carbonaceous c-type asteroid.lightcurve analysis gave a rotation period of 13.577 hours with a brightness variation of 0.16 magnitude (u=3-).in january 2014, photometric observations at the palomar transient factory in california gave a period of 13.583 hours and an amplitude of 0.15 magnitude (u=2).the official naming citation was published in the planetenzirkular des astronomischen rechen-institut (ri 789).

1099 figneria | epoch | 2006-12-31 <tsp> 1099 figneria | orbitalperiod | 1799420000 <tsp> 1099 figneria | periapsis | 3492060000000 <tsp> 1099 figneria | apoapsis | 6057180000 kilometres

1099 Figneria, provisional designation 1928 RQ, is an asteroid from the background population of the outer regions of the asteroid belt, approximately 26 kilometers in diameter.

1099 figneria, provisional designation 1928 rq, is an asteroid from the background population of the outer regions of the asteroid belt, approximately 26 kilometers in diameter.discovered by grigory neujmin at simeiz observatory in 1928, the asteroid was later named after russian revolutionary activist vera figner.on the same night, it was independently discovered by german astronomer max wolf at the heidelberg observatory in southwest germany.the minor planet center, however, only acknowledges the first discoverer.in october 1927, the asteroid was first identified as a917 uf at simeiz, where the body's observation arc begins 11 months later with its official discovery observation.it orbits the sun in the outer main belt at a distance of 2.3–4.1 au once every 5 years and 8 months (2,071 days).its orbit has an eccentricity of 0.28 and an inclination of 12° with respect to the ecliptic.the asteroid is also an assumed carbonaceous c-type asteroid.lightcurve analysis gave a rotation period of 13.577 hours with a brightness variation of 0.16 magnitude (u=3-).in january 2014, photometric observations at the palomar transient factory in california gave a period of 13.583 hours and an amplitude of 0.15 magnitude (u=2).the official naming citation was published in the planetenzirkular des astronomischen rechen-institut (ri 789).

1099 figneria | epoch | 2006-12-31 <tsp> 1099 figneria | orbitalperiod | 1799420000 <tsp> 1099 figneria | periapsis | 3492060000000 <tsp> 1099 figneria | apoapsis | 6057180000 kilometres

1099 Figneria, provisional designation 1928 RQ, is an asteroid from the background population of the outer regions of the asteroid belt, approximately 26 kilometers in diameter.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | escapevelocity | 00473 kilometreperseconds <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | escapevelocity | 00473 kilometreperseconds <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | escapevelocity | 00473 kilometreperseconds <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | escapevelocity | 00473 kilometreperseconds <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | escapevelocity | 00473 kilometreperseconds <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | escapevelocity | 00473 kilometreperseconds <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | periapsis | 2833260000000

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | periapsis | 2833260000000

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | mass | 75 kilograms <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | periapsis | 2833260000000

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | periapsis | 2833260000000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | periapsis | 2833260000000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

felicitas (minor planet designation: 109 felicitas) is a dark and fairly large main-belt asteroid.it was discovered by german-american astronomer c. h. f. peters on october 9, 1869, and named after felicitas, the roman goddess of success.the only observed stellar occultation by felicitas is one from japan (march 29, 2003).this body is orbiting the sun with a period of 4.43 years and an eccentricity (ovalness) of 0.3.its orbital plane is inclined by 7.9° from the plane of the ecliptic.109 felicitas is classified as a carbonaceous gc-type asteroid.it is spinning with a rotation period of 13.2 hours.during 2002, 109 felicitas was observed by radar from the arecibo observatory.the return signal matched an effective diameter of 89 ± 9 km.this is consistent with the asteroid dimensions computed through other means.

109 felicitas | epoch | 2006-12-31 <tsp> 109 felicitas | orbitalperiod | 1397050000 <tsp> 109 felicitas | periapsis | 2833260000000 <tsp> 109 felicitas | apoapsis | 5233290000 kilometres

Felicitas (minor planet designation: 109 Felicitas) is a dark and fairly large main-belt asteroid.109 Felicitas is classified as a carbonaceous GC-type asteroid.During 2002, 109 Felicitas was observed by radar from the Arecibo Observatory.

1101 clematis is an alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.it was discovered on 22 september 1928, by german astronomer karl reinmuth at the heidelberg-königstuhl state observatory in southwest germany, and assigned the provisional designation 1928 sj.it was named for the flowering plant clematis.the presumably carbonaceous asteroid has a relatively long rotation period of 34.3 hours.: 23  according to a different study, this object is also the namesake of the clematis family, a small family of 5–16 asteroids hence they may have arisen from the same collisional event.all members have a relatively high orbital inclination.it orbits the sun in the outermost asteroid belt at a distance of 3.0–3.5 au once every 5 years and 10 months (2,120 days; semi-major axis of 3.23 au).its orbit has an eccentricity of 0.08 and an inclination of 21° with respect to the ecliptic.the body's observation arc begins with its observation as 1963 tg1 at goethe link observatory in october 1963, more than 35 years after its official discovery observation at heidelberg.: 23  === rotation period === in september 2009, a rotational lightcurve of clematis was obtained from photometric observations by american astronomers brian warner at the palmer divide observatory, colorado, and by robert stephens at gmars (g79, california.lightcurve analysis gave a synodic rotation period of 34.3 hours with a brightness amplitude of 0.16 magnitude (u=2), which significantly differs from previously reported periods of 6 to 12.68 hours (u=1/2/2/2).while not being a slow rotator, clematis has a much longer period than that known for most other asteroids, and its small amplitude is indicative for a rather spheroidal shape.the official naming citation was mentioned in the names of the minor planets by paul herget in 1955 (h n.a.).

1101 clematis | epoch | 2006-12-31 <tsp> 1101 clematis | mass | 57 kilograms <tsp> 1101 clematis | orbitalperiod | 1833090000 <tsp> 1101 clematis | apoapsis | 5209060000 kilometres

1101 Clematis is an Alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.

1101 clematis is an alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.it was discovered on 22 september 1928, by german astronomer karl reinmuth at the heidelberg-königstuhl state observatory in southwest germany, and assigned the provisional designation 1928 sj.it was named for the flowering plant clematis.the presumably carbonaceous asteroid has a relatively long rotation period of 34.3 hours.: 23  according to a different study, this object is also the namesake of the clematis family, a small family of 5–16 asteroids hence they may have arisen from the same collisional event.all members have a relatively high orbital inclination.it orbits the sun in the outermost asteroid belt at a distance of 3.0–3.5 au once every 5 years and 10 months (2,120 days; semi-major axis of 3.23 au).its orbit has an eccentricity of 0.08 and an inclination of 21° with respect to the ecliptic.the body's observation arc begins with its observation as 1963 tg1 at goethe link observatory in october 1963, more than 35 years after its official discovery observation at heidelberg.: 23  === rotation period === in september 2009, a rotational lightcurve of clematis was obtained from photometric observations by american astronomers brian warner at the palmer divide observatory, colorado, and by robert stephens at gmars (g79, california.lightcurve analysis gave a synodic rotation period of 34.3 hours with a brightness amplitude of 0.16 magnitude (u=2), which significantly differs from previously reported periods of 6 to 12.68 hours (u=1/2/2/2).while not being a slow rotator, clematis has a much longer period than that known for most other asteroids, and its small amplitude is indicative for a rather spheroidal shape.the official naming citation was mentioned in the names of the minor planets by paul herget in 1955 (h n.a.).

1101 clematis | epoch | 2006-12-31 <tsp> 1101 clematis | mass | 57 kilograms <tsp> 1101 clematis | orbitalperiod | 1833090000 <tsp> 1101 clematis | apoapsis | 5209060000 kilometres

1101 Clematis is an Alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.

1101 clematis is an alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.it was discovered on 22 september 1928, by german astronomer karl reinmuth at the heidelberg-königstuhl state observatory in southwest germany, and assigned the provisional designation 1928 sj.it was named for the flowering plant clematis.the presumably carbonaceous asteroid has a relatively long rotation period of 34.3 hours.: 23  according to a different study, this object is also the namesake of the clematis family, a small family of 5–16 asteroids hence they may have arisen from the same collisional event.all members have a relatively high orbital inclination.it orbits the sun in the outermost asteroid belt at a distance of 3.0–3.5 au once every 5 years and 10 months (2,120 days; semi-major axis of 3.23 au).its orbit has an eccentricity of 0.08 and an inclination of 21° with respect to the ecliptic.the body's observation arc begins with its observation as 1963 tg1 at goethe link observatory in october 1963, more than 35 years after its official discovery observation at heidelberg.: 23  === rotation period === in september 2009, a rotational lightcurve of clematis was obtained from photometric observations by american astronomers brian warner at the palmer divide observatory, colorado, and by robert stephens at gmars (g79, california.lightcurve analysis gave a synodic rotation period of 34.3 hours with a brightness amplitude of 0.16 magnitude (u=2), which significantly differs from previously reported periods of 6 to 12.68 hours (u=1/2/2/2).while not being a slow rotator, clematis has a much longer period than that known for most other asteroids, and its small amplitude is indicative for a rather spheroidal shape.the official naming citation was mentioned in the names of the minor planets by paul herget in 1955 (h n.a.).

1101 clematis | epoch | 2006-12-31 <tsp> 1101 clematis | mass | 57 kilograms <tsp> 1101 clematis | orbitalperiod | 1833090000 <tsp> 1101 clematis | apoapsis | 5209060000 kilometres

1101 Clematis is an Alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.

amsterdamsche football club ajax (dutch pronunciation: [ˈaːjɑks]), also known as afc ajax, ajax amsterdam, or simply ajax, is a dutch professional football club based in amsterdam, that plays in the eredivisiecode: nld promoted to code: nl , the top tier in dutch football.historically, ajax (named after the legendary greek hero) is the most successful club in the netherlands, with 36 eredivisie titlescode: nld promoted to code: nl and 20 knvb cups.it has continuously played in the eredivisiecode: nld promoted to code: nl , since the league's inception in 1956 and, along with feyenoordcode: nld promoted to code: nl and psv eindhovencode: nld promoted to code: nl , it is one of the country's 'big three' clubs that have dominated that competition.ajax was one of the most successful clubs in the world in the 20th century.according to the international federation of football history & statistics, ajax was the seventh-most successful european club of the 20th century and the world's club team of the year in 1992.according to german magazine kicker, ajax was the second-most successful european club of the 20th century.the club is one of five teams that have earned the right to keep the european cup and to wear a multiple-winner badge.in 1972, they completed the continental treble by winning the eredivisiecode: nld promoted to code: nl , knvb cup, and the european cup.they also won the first (albeit unofficial) european super cup against rangers in january 1973.ajax's most recent international trophies are the 1995 intercontinental cup, 1995 uefa super cup and the 1995 champions league, where they defeated milan in the final; they lost the 1996 champions league final on penalties to juventus.in 1995, ajax was crowned as world team of the year by world soccer magazine.ajax is also one of four teams to win the continental treble and the intercontinental cup or club world cup in the same season/calendar year; this was achieved in the 1971–72 season.

afc ajax | manager | frank de boer <tsp> frank de boer | club | al-shamal sports club <tsp> frank de boer | club | fc barcelona <tsp> frank de boer | club | netherlands national football team

Amsterdamsche Football Club Ajax (Dutch pronunciation: [ˈaːjɑks]), also known as AFC Ajax, Ajax Amsterdam, or simply Ajax, is a Dutch professional football club based in Amsterdam, that plays in the Eredivisiecode: nld promoted to code: nl , the top tier in Dutch football.Historically, Ajax (named after the legendary Greek hero) is the most successful club in the Netherlands, with 36 Eredivisie titlescode: nld promoted to code: nl and 20 KNVB Cups.It has continuously played in the Eredivisiecode: nld promoted to code: nl , since the league's inception in 1956 and, along with Feyenoordcode: nld promoted to code: nl and PSV Eindhovencode: nld promoted to code: nl , it is one of the country's 'big three' clubs that have dominated that competition.Ajax was one of the most successful clubs in the world in the 20th century.According to the International Federation of Football History & Statistics, Ajax was the seventh-most successful European club of the 20th century and The World's Club Team of the Year in 1992.According to German magazine Kicker, Ajax was the second-most successful European club of the 20th century.The club is one of five teams that have earned the right to keep the European Cup and to wear a multiple-winner badge.Ajax's most recent international trophies are the 1995 Intercontinental Cup, 1995 UEFA Super Cup and the 1995 Champions League, where they defeated Milan in the final; they lost the 1996 Champions League final on penalties to Juventus.Ajax is also one of four teams to win the continental treble and the Intercontinental Cup or Club World Cup in the same season/calendar year; this was achieved in the 1971–72 season'