Across much of the world, the open star cluster IC 2395 (mag 4.0) in Vela will be well placed in the evening sky in coming weeks. On 1 February it will reach its highest point in the sky at around midnight local time, and on subsequent evenings it will culminate four minutes earlier each day.
From South El Monte , however, it is not readily observable since it lies so far south that it will never rise more than 7° above the horizon.
At a declination of 48°09'S, it is easiest to see from the southern hemisphere but cannot be seen from latitudes much north of 21°N.
At magnitude 4.0, IC2395 is tricky to make out with the naked eye except from a dark site, but is visible through a pair of binoculars or small telescope.
The position of IC2395 is as follows:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| IC2395 | 08h42m30s | 48°09'S | Vela | 4.0 | 6'00" |
The coordinates above are given in J2000.0.
The sky on 30 Jun 2025
| The sky on 30 June 2025 | ||||||||||||||||||||||||||||||||||
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36% 5 days old |
All times shown in PDT.
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Source
The circumstances of this event were computed using the DE430 planetary ephemeris published by the Jet Propulsion Laboratory (JPL).
This event was automatically generated by searching the ephemeris for planetary alignments which are of interest to amateur astronomers, and the text above was generated based on an estimate of your location.
Image credit
© Digitised Sky Survey (DSS); Second Palomar Observatory Sky Survey (POSS-II)