SpaceTRCSpaceTRC/Research platform
TürkçeLet’s collaborate
SpaceTRC / Cosmos / Constellations

Lupus (Wolf)

COSMOS / CONSTELLATIONS / LUP

Lupus (Wolf)

The Wolf. IAU abbreviation Lup. One of the 48 classical constellations listed by Ptolemy in the Almagest in the 2nd century AD.

STAR CHART

α Lupβ Lupγ Lupδ Lupε Lupζ Lup↑ N ← E
Coloured dots are the stars of Lupus brighter than magnitude 6.5 (size by brightness, colour by temperature); grey dots are stars brighter than 5.5 in neighbouring constellations. North is up, east to the left. Constellation boundaries and traditional stick figures are not drawn.

KEY FACTS

IAU abbreviation
Lup
Latin name / genitive
Lupus / Lupi
Position
Right ascension ≈ 15 h 15 m; declination −55° to −30°
Visibility from Türkiye
From Türkiye only its northern part is seen, low on the southern horizon; the southern provinces are better placed.
Best time to observe
Best placed at 21:00 Türkiye time around 7 July.
Number of stars
124 stars brighter than magnitude 6.5 in the catalogue; 34 brighter than 5 and 12 brighter than 4.

INTERACTIVE LAB

Where is Lupus tonight?

Only the northern part of this constellation is seen from Türkiye, low on the southern horizon. The lab opens for Ankara on today’s date; switch the city to Antalya and then to Sydney and watch how the “Visible part” row and the chart change. The “Best night” button jumps to the best date (around 7 July).

MYTH, HISTORY AND OBSERVING

Ptolemy described it simply as a wild animal; later it became a wolf, drawn impaled on the spear of Centaurus. SN 1006, the brightest supernova in recorded history, appeared here in the year 1006. From Türkiye it is partly visible low in the south in early summer.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
α Lup2.30465B1.5III
β Lup2.68383B2III
γ Lup2.80421B2IV
δ Lup3.22884B1.5IV
ε Lup3.37512B2IV-V
ζ Lup3.41117G8III
η Lup3.42442B2.5IV
ι Lup3.55338B2.5IV

Magnitude: apparent brightness; the smaller the number, the brighter the star. Distances derive from parallax measurements and are uncertain for distant stars. Source: HYG v4.1 star catalogue (CC BY-SA 4.0).

SOURCES

Position, visibility and best observing time were computed approximately for this page from the catalogue stars (Ankara, 39.9° N). The 88 constellations were adopted by the IAU in 1922; their boundaries were drawn by Eugène Delporte in 1930.

SPACETRC / KNOWLEDGE

Follow your curiosity.

SPACETRC / GET STARTED

What would you like to do?

This short guide is available in six languages. Full scientific articles are in Turkish and English.

Open a workspace

Search publicationsExamine dataSpace eventsPlan a team projectPrepare a publication

Take selected reading with you

Open Turkish and English dossiers and introductory lessons in the reading area. Offline preparation and installation options are available there.

Open the offline library ↗

The language preference stays in this browser; no account or location permission is required.