I have received an update to the recent outburst of RS Ophiuchi to naked eye levels (mag 4.8). This recurrent nova has not outburst to naked eye levels since 1985. If it dims according to past observations, it should lose about 0.1 magnitudes a day for about a month, returning to normal in about 110 days.
For those that may want to look the star up with planetarium software, Starry Night Pro does not list RS Oph in its variable database. However a similar star in the vicinity with the same J2000 co-ordinates is TYC5094-550-1.
According to the AAVSO ?A? level chart (1744-06A), RS Oph is almost midway on an imaginary line between the globular cluster M14 and M16, the Eagle Nebula. It should be possible to frame M14 with RS Oph in a pair of 7×35 binoculars!
The original Special Notice #6 concerning RS Oph is listed at this link:
http://www.aavso.org/publications/specialnotice/6.shtml
The update was released as Alert Notice #335 and is available at this link:
http://www.aavso.org/publications/alerts/alert335.shtml
Charts for this recurrent nova are available at this link:
http://www.aavso.org/cgi-bin/searchcharts3.pl?name=rs%20oph
Variable star observing is a fun and rewarding aspect of amateur astronomy and is one of the many ways that amateurs can contribute to real science. Unlike supernova hunts or astro-imaging, it does not require a great deal of hardware to start; a pair of binoculars or small telescope will do just fine.
