六月牧夫座流星雨也称为天龙座ι流星雨,与彗星7P/庞士-温尼克彗星相关联,最早是在1916年5月27日被威廉F丹宁确认[28]。这个流星雨,流星的速度缓慢,在1916年之前没有被观测的资料。因为在之前地球并未穿越这颗彗星的尘埃尾,直到7P/庞士-温尼克彗星的轨道受到木星的摄动,造成它的与地球轨道接近至0.03AU,而首度观测到六月牧夫座流星雨。在1982年,E. A. Reznikov发现1916年的爆发是1819年的彗星释放出来的物质[29]。但因为7P/庞士-温尼克彗星的轨道不在适合的位置上,直到1998年才再度观察到另一次的爆发。不过,1998年6月27日的流星雨辐射点在牧夫座,稍后被证实为7P/庞士-温尼克彗星相关。这些流星令人难以置信的长寿,最亮的流星痕迹持续了数秒钟的时间。各地观察到的爆发,有许多的火球拖着长长的绿色尾迹,甚至投下一些阴影,最大的天顶每小时流星数达到每小时200-300颗流星[30]。在2002年,两位俄罗斯天文徐家确认这颗彗星在1825年的喷发造成了1998年的爆发[31],并预期来自1819年、1825年和1830年喷发的颗粒会在2004年6月23日进入地球的大气层。预期中的流星雨不如1998年的壮观,被证实的每小时天顶流星数是每小时16-20颗的流星。预测在未来的50年内,六月牧夫座流星雨不会有特别显著的爆发[32]。在通常情况下,每小时只能看见1-2颗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。它们是由天龙座α和牧夫座-天龙座释出。这个流星雨从6月27日持续至7月5日,极大期落在6月28日[33]。六月牧夫座流星雨属于第三集的流星雨(变化无常)[34],进入的平均速度是18公/秒,辐射点在牧夫座β星北方约7度[35]。
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