六月牧夫座流星雨也稱為天龍座ι流星雨,與彗星7P/龐士-溫尼克彗星相關聯,最早是在1916年5月27日被威廉F丹寧確認[28]。這個流星雨,流星的速度緩慢,在1916年之前沒有被觀測的資料。因為在之前地球並未穿越這顆彗星的塵埃尾,直到7P/龐士-溫尼克彗星的軌道受到木星的攝動,造成它的與地球軌道接近至0.03AU,而首度觀測到六月牧夫座流星雨。在1982年,E. A. Reznikov發現1916年的爆發是1819年的彗星釋放出來的物質[29]。但因為7P/龐士-溫尼克彗星的軌道不在適合的位置上,直到1998年才再度觀察到另一次的爆發。不過,1998年6月27日的流星雨輻射點在牧夫座,稍後被證實為7P/龐士-溫尼克彗星相關。這些流星令人難以置信的長壽,最亮的流星痕跡持續了數秒鐘的時間。各地觀察到的爆發,有許多的火球拖着長長的綠色尾跡,甚至投下一些陰影,最大的天頂每小時流星數達到每小時200-300顆流星[30]。在2002年,兩位俄羅斯天文徐家確認這顆彗星在1825年的噴發造成了1998年的爆發[31],並預期來自1819年、1825年和1830年噴發的顆粒會在2004年6月23日進入地球的大氣層。預期中的流星雨不如1998年的壯觀,被證實的每小時天頂流星數是每小時16-20顆的流星。預測在未來的50年內,六月牧夫座流星雨不會有特別顯著的爆發[32]。在通常情況下,每小時只能看見1-2顆度很慢且黯淡的流星;六月牧夫座流星雨的平均星等是5.0。它們是由天龍座α和牧夫座-天龍座釋出。這個流星雨從6月27日持續至7月5日,極大期落在6月28日[33]。六月牧夫座流星雨屬於第三集的流星雨(變化無常)[34],進入的平均速度是18公/秒,輻射點在牧夫座β星北方約7度[35]。
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