Similarities between 1063 Aquilegia and List of minor planets: 1001–2000
1063 Aquilegia and List of minor planets: 1001–2000 have 4 things in common (in Unionpedia): Heidelberg-Königstuhl State Observatory, Karl Wilhelm Reinmuth, List of minor planet discoverers, 1054 Forsytia.
Heidelberg-Königstuhl State Observatory
Heidelberg-Königstuhl State Observatory (Landessternwarte Heidelberg-Königstuhl) is a historic astronomical observatory located near the summit of the Königstuhl hill in the city of Heidelberg in Germany.
1063 Aquilegia and Heidelberg-Königstuhl State Observatory · Heidelberg-Königstuhl State Observatory and List of minor planets: 1001–2000 ·
Karl Wilhelm Reinmuth
Karl Wilhelm Reinmuth (April 4, 1892 in Heidelberg – May 6, 1979 in Heidelberg) was a German astronomer and a prolific discoverer of 395 minor planets.
1063 Aquilegia and Karl Wilhelm Reinmuth · Karl Wilhelm Reinmuth and List of minor planets: 1001–2000 ·
List of minor planet discoverers
This is a list of all astronomers who are credited by the Minor Planet Center (MPC) with the discovery of one or several minor planets.
1063 Aquilegia and List of minor planet discoverers · List of minor planet discoverers and List of minor planets: 1001–2000 ·
1054 Forsytia
1054 Forsytia, provisional designation, is a dark background asteroid from the outer regions of the asteroid belt, approximately 46 kilometers in diameter.
1054 Forsytia and 1063 Aquilegia · 1054 Forsytia and List of minor planets: 1001–2000 ·
The list above answers the following questions
- What 1063 Aquilegia and List of minor planets: 1001–2000 have in common
- What are the similarities between 1063 Aquilegia and List of minor planets: 1001–2000
1063 Aquilegia and List of minor planets: 1001–2000 Comparison
1063 Aquilegia has 41 relations, while List of minor planets: 1001–2000 has 859. As they have in common 4, the Jaccard index is 0.44% = 4 / (41 + 859).
References
This article shows the relationship between 1063 Aquilegia and List of minor planets: 1001–2000. To access each article from which the information was extracted, please visit: