Brocchi's Cluster
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Brocchi's Cluster
Summary
Brocchi's Cluster is a star cluster[1]. It draws 882 Wikipedia views per month (star_cluster category, ranking #1,838 of 43).[2]
Key Facts
- Brocchi's Cluster is credited with the discovery of Abd al-Rahman al-Sufi[3].
- Brocchi's Cluster's instance of is recorded as star cluster[4].
- Brocchi's Cluster's constellation is recorded as Vulpecula[5].
- Brocchi's Cluster's Commons category is recorded as Coathanger Cluster[6].
- Brocchi's Cluster's catalog code is recorded as OCl 113[7].
- Brocchi's Cluster's catalog code is recorded as OCl 113.0[8].
- Brocchi's Cluster's catalog code is recorded as C 1923+200[9].
- Brocchi's Cluster's time of discovery or invention is recorded as 964[10].
- Brocchi's Cluster's apparent magnitude is recorded as {'amount': '+3.93'}[11].
- Brocchi's Cluster's apparent magnitude is recorded as {'amount': '+3.6'}[12].
- Brocchi's Cluster's right ascension is recorded as {'amount': '+291.350'}[13].
- Brocchi's Cluster's declination is recorded as {'amount': '+20.183'}[14].
- Brocchi's Cluster's epoch is recorded as J2000.0[15].
Body
Definition and Type
Brocchi's Cluster's instance of is recorded as star cluster[4].
Why It Matters
Brocchi's Cluster draws 882 Wikipedia views per month (star_cluster category, ranking #1,838 of 43).[2] It has Wikipedia articles in 15 language editions, a strong signal of global cultural recognition.[16] It is known by 22 alternative names across languages and contexts.[17]