A spiral galaxy in Canes Venatici, named for the many short arms its photographs show. Maps of its starlight and its gas weigh what it shines with: about a fifth of that is still gas, the raw material for new stars.
Galaxy in Canes Venatici. Magnitude 8.6.
From Georgetown (6.8° N) it climbs to 55° above the northern horizon at its highest; from Lethem (3.4° N), to 52° above the northern horizon. It is highest at midnight on the night of 8 Apr, in the middle of its season. The page works out tonight's rise, highest point and set for both towns in Guyana time (UTC-4), and where the Moon is.
Apparent size from OpenNGC (Mattia Verga), CC-BY-SA-4.0.
Measured: What its visible mass is made of: stars and gas, not dark matter.
Each mass is given to a tenth of a dex, so each share is good to about a quarter of itself. Dark matter is not counted. Leroy et al. 2008, AJ 136, 2782, Table 4 (VizieR J/AJ/136/2782), NGC 5055: log stellar mass 10.8, atomic gas 10.1, molecular gas 9.7 (Suns). Shares do not depend on the distance the paper adopted.
Also in it, not measured:
How we know: Distance from its brightest red giants (the tip of the red giant branch): NED-D (NASA/IPAC Extragalactic Database, redshift-independent distances), median of 2 TRGB estimates: 9.09 Mpc, 8.87-9.32 Mpc; e.g. 2017AJ....154...51M, 2015AstL...41..239T; retrieved 2026-10-21. True size: the apparent size times the distance (apparent size: OpenNGC (Mattia Verga, CC BY-SA 4.0), commit 4e2398a2).

More deep-sky objects: M94 (Galaxy) · Whirlpool Galaxy (M51) · Galaxy M106 · Pinwheel Galaxy (M101) · M109 (Galaxy) · Needle Galaxy (NGC 4565)