|Help and Advice|
|Transit of Mercury 2016|
|Giving long exposures on a digital camera|
|Photographing star trails|
|Predicting the ISS and other satellites|
|Using a mirror to view a partial eclipse|
|Simple Guide to Viewing the Space Station|
|Choosing a Telescope|
|Tips when projecting the Sun|
|Starting to Use Your Telescope|
|Imaging with a DSLR through the telescope|
|Buying a telescope for a child|
|Photographing a partial eclipse|
|Main Activity Dates||June 22 - July 2|
|Peak Rates||June 23-24?|
|Peak ZHR||usually low, occasional outbursts|
|Best Observed Rates||?|
|Visibility each night (UK)||Visible all night|
|Moonlight issues at Maximum||None - New Moon is on June 24|
The June Bootids are an unpredictable source.
They produced an unexpected outburst on 1998 June 27, when ZHRs of 50-100+ were observed for over 12 hours, with rates seen on just one date. Before this, only three returns of the shower were known, from 1916, 1921 and 1927.
Another ZHR ~50 outburst happened on 2004 June 23, but a similar event predicted for 2010 June 23/24 proved disappointingly very weak.
The shower is associated with Comet 7P/Pons-Winnecke. This last passed through perihelion on 2015 January 30. However, whereas enhanced activity from other meteor showers has been most likely to occur when their parent comet is near perihelion, there seems to have been no such correlation regarding previous outbursts of the June Bootids.
Moonlight will not be an issue - New Moon in 2017 is on June 24. A more significant issue will of course be Britain's short, twilit midsummer nights - although even casual observers here easily spotted the 1998 return.
No activity is expected this year, though recent IMO video results have indicated very weak rates may happen annually from the shower, on or around June 24, so it is worth keeping watch then just in case, and also around the 1998 peak's repeat time, on June 27. The June 24 video June Boötids were radiating from an area about 10° south of the expected one, however.
June Bootids are typically very slow meteors - a factor which helps distinguish them from sporadic meteors which might by chance line up with the radiant.
The chart below shows the radiant location as reported in 1998: