Here is a fun and easy Lyra observing project I started last week. It can be done with a hand held binocular (if you insist).
Beta Lyrae, aka Sheliak, is a remarkable eclipsing binary star about 960 light years away. It varies in magnitude between 3.25 and 4.36 in a period of 12.9 days. What causes the change in magnitude is that mass has been transferred from what was originally the larger star of the spectroscopic binary pair to the companion star, forming a torus ring around the companion which shrouds its light, making it dimmer. A helpful visualization can be viewed in this Texas A&M astronomy department archive. When the secondary (spectroscopic companion star) is fully in front of the primary, Sheliak's magnitude is at its minimum of 4.36. When the primary star is fully in front of the secondary, Sheliak is at its 3.25 maximum.
What makes it a particularly easy variable star to follow is that the adjacent Lyra asterism p-gram stars provide convenient magnitude references.
Sulafat (southeast corner) is 3.25 magnitude, which is Sheliak's maximum and Zeta1 Lyrae is 4.34 magnitude, close to Sheliak's minimum.
Last Wednesday night (28 June 2023) Sheliak was not quite as bright as Sulafat, but obviously brighter than Zeta1. Friday evening (30 June) Sheliak seemed slightly fainter -- still brighter than Zeta1, but not as close in brightness to Sulafat. It was cloudy and raining last night, so I wasn't able to observe it. But the next evening it is clear I'll take another look to see if its magnitude is declining now.
An observation like this can be made in a minute or two, easily accomplished any clear evening.