Djorgovski 1

{{Infobox globular cluster

| name = Djorgovski 1

| image = 250px

| epoch = J2000

| ra = {{RA|17|47|28.3}}{{cite web |title=Djorg 1 |url=http://spider.seds.org/spider/MWGC/djorg1.html |website=Spider.SEDS.org |accessdate=19 June 2015 |archiveurl=https://web.archive.org/web/20160304134159/http://spider.seds.org/spider/MWGC/djorg1.html |archivedate=4 March 2016 |url-status=dead }}

| dec = {{DEC|-33|03:56}}

| dist_ly =44.7 kly

| appmag_v = 13.6

| constellation = Scorpius

| metal_fe = −1.51{{cite web |last1=Valenti |first1=Elena |last2=Ferraro |first2=Francesco R |last3=Origlia |first3=Livia |title=Near-IR Properties of Globular Clusters in the Galactic Bulge |url=http://www.bo.astro.it/~GC/ir_archive/ |accessdate=19 June 2015 |archiveurl=https://web.archive.org/web/20150923192842/http://www.bo.astro.it/~GC/ir_archive/ |archivedate=23 September 2015 |url-status=dead }}| age =

| names = Djorg 1

}}

Djorgovski 1 is a globular cluster discovered in 1986 by George Djorgovski who was looking for possible obscured globular clusters using the IRAS Point Source Catalog.{{cite journal |last1=Djorgovski |first1=S |title=Discovery of three obscured globular clusters |journal=The Astrophysical Journal |volume=317 |pages=L13 |bibcode=1987ApJ...317L..13D |doi=10.1086/184903|year=1987 |url=https://authors.library.caltech.edu/97628/1/1987ApJ___317L__13D.pdf }} Studies show that its stars are "metal-poor" – they contain hydrogen and helium but little else. Djorgovski 1 is actually one of the most metal-poor clusters in the inner galaxy.{{cite web |title=Engulfed by stars near the Milky Way's heart |url=https://www.spacetelescope.org/images/potw1126a/ |website=Hubble Space telescope |accessdate=19 June 2015 |archiveurl=https://web.archive.org/web/20150619153933/https://www.spacetelescope.org/images/potw1126a/ |archivedate=19 June 2015 |url-status=dead }}