M90
NGC 4569 · Galaxy in Virgo
- Magnitude
- 9.5
- Size
- 9.5′ × 4.5′
- Effective surface brightness
- 22.2 mag/arcsec²
- Best months
- Mar, Apr, May
- Declination
- +13°
- Filter
- None (broadband target)
A large spiral whose arms have been stripped by the cluster medium. Smooth and elongated.
Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.
How long with each smart telescope
| Telescope | In frame | Bortle 3 (rural) | Bortle 5 (suburban) | Bortle 7 (urban edge) |
|---|---|---|---|---|
| ZWO Seestar S5010 s subs | 22% | 58 min351 subs | 1 h 36 min574 subs | 4 h 18 min1,551 subs |
| ZWO Seestar S50 Pro10 s subs | 11% | 1 h 05 min391 subs | 1 h 45 min632 subs | 4 h 41 min1,688 subs |
| ZWO Seestar S3010 s subs | 13% | 1 h 06 min397 subs | 1 h 43 min620 subs | 4 h 26 min1,597 subs |
| ZWO Seestar S30 Pro10 s subs | 7% | 1 h 10 min419 subs | 1 h 52 min673 subs | 4 h 57 min1,784 subs |
| DwarfLab DWARF 315 s subs | 10% | 1 h 16 min305 subs | 2 h 14 min535 subs | 6 h 25 min1,541 subs |
| DwarfLab DWARF mini15 s subs | 13% | 58 min231 subs | 1 h 35 min380 subs | 4 h 18 min1,031 subs |
| DwarfLab Draco30 s subs | 13% | 47 min94 subs | 1 h 18 min156 subs | 3 h 33 min427 subs |
| DwarfLab DWARF II15 s subs | 9% | 4 h 20 min1,042 subs | 6 h 04 min1,455 subs | 14 h3,263 subs |
| Vaonis Vespera II10 s subs | 11% | 58 min351 subs | 1 h 36 min574 subs | 4 h 18 min1,551 subs |
| Vaonis Vespera Pro10 s subs | 10% | 2 h 24 min862 subs | 3 h 42 min1,332 subs | 9 h 24 min3,385 subs |
| Vaonis Vespera 310 s subs | 11% | 55 min332 subs | 1 h 31 min547 subs | 4 h 07 min1,485 subs |
| Vaonis Vespera Pro 210 s subs | 10% | 2 h 15 min813 subs | 3 h 31 min1,264 subs | 8 h 59 min3,236 subs |
| Unistellar eQuinox 24 s subs | 28% | 1 h 20 min1,195 subs | 1 h 43 min1,543 subs | 3 h 24 min3,064 subs |
| Unistellar Odyssey4 s subs | 28% | 7 h 06 min6,389 subs | 8 h 30 min7,655 subs | 15 h13,191 subs |
| Celestron Origin10 s subs | 19% | 14 min82 subs | 24 min146 subs | 1 h 10 min423 subs |
| Celestron Origin Mark II10 s subs | 21% | 17 min102 subs | 32 min193 subs | 1 h 39 min592 subs |
Imaging the galaxy
Galaxies are broadband targets: their light is mostly starlight spread across the spectrum, so a dual-band filter throws most of it away and makes things slower, not faster. Shoot without a filter (or with a plain UV/IR cut) and rely on total time and a dark sky. The core of a galaxy is usually many times brighter than its outer disc, so a short stack shows the nucleus long before the arms; the figures here are for the arms and disc, not the core.
Field rotation in Alt-Az mode crops the edges of the stack over a long session, so on a big galaxy re-centre now and then or use EQ mode where your scope supports it.
Per-telescope pages
- How long to image the M90 with the ZWO Seestar S50
- How long to image the M90 with the ZWO Seestar S50 Pro
- How long to image the M90 with the ZWO Seestar S30
- How long to image the M90 with the ZWO Seestar S30 Pro
- How long to image the M90 with the DwarfLab DWARF 3
- How long to image the M90 with the DwarfLab DWARF mini
- How long to image the M90 with the DwarfLab Draco
- How long to image the M90 with the DwarfLab DWARF II
- How long to image the M90 with the Vaonis Vespera II
- How long to image the M90 with the Vaonis Vespera Pro
- How long to image the M90 with the Vaonis Vespera 3
- How long to image the M90 with the Vaonis Vespera Pro 2
- How long to image the M90 with the Unistellar eQuinox 2
- How long to image the M90 with the Unistellar Odyssey
- How long to image the M90 with the Celestron Origin
- How long to image the M90 with the Celestron Origin Mark II