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False Cross

Naked Eye • Asterisms False Cross finder map.

Finder map for False Cross

A well-known “false Southern Cross” in modern celestial navigation and observational lore. Unlike the true Southern Cross (Crux), it has no established mythological or cultural significance and is primarily noted as a navigational look-alike in the southern sky. Best viewed from southern latitudes, where it rises high in the sky. From low northern latitudes it remains very low above the southern horizon and is easily obscured; it is inaccessible from mid- and high-northern latitudes. The primary challenge for beginners is distinguishing it from the true Southern Cross (Crux).

PropertyValue
Common namesDiamond Cross
Catalog names-
TypeAsterism
Subtype-
Coordinates08h 57m 04.7s, -57° 16’ 23.6”
SeasonJanuary - March
Best monthFebruary
Beginner friendlyYes
Visual rewardHigh
Filters requiredNone
LP toleranceMedium
Minimum equipmentNaked eye
Optimal equipmentNaked eye
Magnitude-
Size-
ConstellationMultiple

Observation Notes

Naked Eye

Easily visible from the Southern Hemisphere as a prominent diamond-shaped pattern formed by four bright stars. Because of its shape and orientation, it is sometimes mistaken by beginners for the Southern Cross, though it is larger and lacks the distinctive short crossbar of Crux.

Binoculars

Frames the entire asterism attractively against the rich southern Milky Way. Subtle color differences among the component stars are more noticeable at this scale.

Small Telescope

Far too large to fit in a single field of view. Individual stars can be examined separately; Delta Velorum is a noteworthy multiple star system, though resolving its components depends on aperture and seeing.

Medium Telescope

Allows cleaner separation of Delta Velorum’s brighter components under good conditions. Primarily useful for studying individual stars and the surrounding dense star fields rather than for any nebulous detail.

Large Telescope

Not suitable for viewing the asterism as a whole. Best used for detailed study of the individual stars or for observing unrelated deep-sky objects in the surrounding fields.

Observing False Cross from your latitude

From mid-southern latitudes (~45°S), False Cross reaches a maximum altitude of about 78° above the southern horizon and is circumpolar — it never sets, staying above the horizon all night, best placed February - April.

Your latitudeMax altitudeHours above horizon
60°N (≈ Oslo, Helsinki, Anchorage)Below horizonNever rises
50°N (≈ London, Prague, Vancouver)Below horizonNever rises
40°N (≈ Madrid, New York, Beijing)Below horizonNever rises
30°N (≈ Cairo, Houston, Delhi)3h 49m
20°N (≈ Honolulu, Mexico City, Mumbai)13°7h 35m
10°N (≈ Chennai, Bangalore, Bangkok)23°10h 1m
(≈ Quito, Nairobi, Singapore)33°12h 8m
20°S (≈ Rio de Janeiro, Antananarivo, Alice Springs)53°16h 47m
35°S (≈ Sydney, Cape Town, Buenos Aires)68°Circumpolar (24h)
45°S (≈ Christchurch, Hobart, Puerto Montt)78°Circumpolar (24h)

Altitudes and durations are geometric, computed for each latitude, independent of date. Set your location below for tonight's exact rise, transit, and set times.

Visibility from New York
This object never rises above the horizon from New York.
Altitude
Below horizon
Azimuth
Max Altitude
Below horizon
Rises
Sets
Transit
False Cross: RA 08h 57m 04.7s, Dec -57° 16' 23.6"
Computed for the night of July 13–14, 2026 (New York).