Lepus constellation: how to find it, when to see it and what is in it
In short
Lepus (Lep) is a equatorial constellation covering 290 square degrees, number 51 of 88 by size. Its brightest star is Arneb, a yellow-white supergiant, magnitude 2.6. It is best seen in the evening in January. Over London it rises and sets and is well placed in its season. Its neighbours in the sky: Canis Major, Caelum, Columba, Eridanus, Monoceros, Orion.
Area: 290 square degrees, 51 of 88 · Neighbours: Canis Major, Caelum, Columba, Eridanus, Monoceros, Orion · Updated 10 October 2026
How to find Lepus
- 1
When to look
The best time is in January in the evening: in the south, around 21:56.
- 2
Use the neighbours
Find it from the neighbouring constellations: Canis Major, Caelum, Columba, Eridanus.
- 3
Brightest stars
The brightest stars of the figure: Arneb (2.6ᵐ), Nihal (2.8ᵐ), Ping (3.2ᵐ).
When it is visible over London
| Month | Where and when | Conditions |
|---|---|---|
| January | in the south, around 21:56 | around midnight |
| February | in the south, around 19:44 | in the evening |
| March | in the south, around 19:17 | low, needs an open horizon |
| April — august | — | not visible, behind the Sun |
| September | in the southeast, around 05:13 | low, needs an open horizon |
| October | in the south, around 04:49 | before dawn |
| November — december | in the south, around 01:58 | around midnight |
Stars of the constellation
| Star | What it is | Magnitude |
|---|---|---|
| Arneb · α Lep | yellow-white supergiant | 2.6ᵐ |
| Nihal · β Lep | yellow bright giant | 2.8ᵐ |
| Ping · ε Lep | orange giant | 3.2ᵐ |
| Bade · μ Lep | blue-white giant | 3.3ᵐ |
| Darlugal · ζ Lep | white main-sequence star | 3.5ᵐ |
| γ Lep | yellow-white main-sequence star | 3.6ᵐ |
| η Lep | yellow-white giant | 3.7ᵐ |
| δ Lep | orange giant | 3.8ᵐ |
Lepus FAQ
When is the best time to see Lepus?
Where is Lepus in the sky?
What is the brightest star in Lepus?
Neighbouring and other constellations
Related
Constellation lines: Stellarium, CC BY-SA · star names: IAU WGSN, CC BY 4.0