Across much of the world, the Milky Way's dwarf companion , the Small Magellanic Cloud (SMC; mag 2.7), in Tucana will be well placed in the evening sky in coming weeks. On 4 October 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 Columbus , however, it is not observable because it lies so far south that it never rises above the horizon.
At a declination of 72°48'S, it is easiest to see from the southern hemisphere but cannot be seen from latitudes much north of 2°S.
At magnitude 2.7, SMC is visible to the naked eye, but best viewed through a pair of binoculars.
The position of SMC is as follows:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| SMC | 00h52m30s | 72°48'S | Tucana | 2.7 | 0'00" |
The coordinates above are given in J2000.0.
The sky on 5 Oct 2018
| The sky on 5 October 2018 | ||||||||||||||||||||||||||||||||||
|
15% 26 days old |
All times shown in EDT.
|
|||||||||||||||||||||||||||||||||
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)