Similarities between 2MASS J154043.42-510135.7 and List of nearest stars and brown dwarfs
2MASS J154043.42-510135.7 and List of nearest stars and brown dwarfs have 4 things in common (in Unionpedia): Light-year, Red dwarf, Stellar classification, The Astrophysical Journal.
Light-year
The light-year is a unit of length used to express astronomical distances and measures about 9.5 trillion kilometres or 5.9 trillion miles.
2MASS J154043.42-510135.7 and Light-year · Light-year and List of nearest stars and brown dwarfs ·
Red dwarf
A red dwarf (or M dwarf) is a small and relatively cool star on the main sequence, of M spectral type.
2MASS J154043.42-510135.7 and Red dwarf · List of nearest stars and brown dwarfs and Red dwarf ·
Stellar classification
In astronomy, stellar classification is the classification of stars based on their spectral characteristics.
2MASS J154043.42-510135.7 and Stellar classification · List of nearest stars and brown dwarfs and Stellar classification ·
The Astrophysical Journal
The Astrophysical Journal, often abbreviated ApJ (pronounced "ap jay") in references and speech, is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler.
2MASS J154043.42-510135.7 and The Astrophysical Journal · List of nearest stars and brown dwarfs and The Astrophysical Journal ·
The list above answers the following questions
- What 2MASS J154043.42-510135.7 and List of nearest stars and brown dwarfs have in common
- What are the similarities between 2MASS J154043.42-510135.7 and List of nearest stars and brown dwarfs
2MASS J154043.42-510135.7 and List of nearest stars and brown dwarfs Comparison
2MASS J154043.42-510135.7 has 9 relations, while List of nearest stars and brown dwarfs has 140. As they have in common 4, the Jaccard index is 2.68% = 4 / (9 + 140).
References
This article shows the relationship between 2MASS J154043.42-510135.7 and List of nearest stars and brown dwarfs. To access each article from which the information was extracted, please visit: