Celestial hemisphere:  Southern  ·  Constellation: Ophiuchus (Oph)
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Nova - RS Ophiuchi, Prabhakaran
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Nova - RS Ophiuchi

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Nova - RS Ophiuchi, Prabhakaran
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Nova - RS Ophiuchi

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Description

The recurrent nova RS Ophiuchi (RS Oph), located in the constellation of Ophiuchus, is in a rare outburst, it's first for more than 15 years. RS Oph brightened rapidly on 8 August 2021 from around magnitude +12 to shine presently at about magnitude +4.8, a 600-fold in just a day. This is its first outburst since February 2006 and only five other eruptions have been observed since 1898.


RS Oph is a cataclysmic variable star that’s further classified as belonging to a much smaller subset called recurrent novae. This is a very exclusive club, as there are just seven such systems. RS Oph is a binary star system, where a class M2 red giant star is losing material to a compact and dense white dwarf remnant. Every so often the white dwarf flings off this unwanted material in a nuclear blast, causing a huge and rapid brightening. Recurrent novae outburst occasionally between periods of tens to hundreds of years. Classical novae, such as the recent Nova Cas 2021 and Nova Her 2021, on the other hand, exhibit one massive eruption, or outburst, with the progenitor system brightening by between 8 to 15 magnitudes before slowly fading to its quiescence state.


Unlike classical novae, astronomers can predict with a good deal of accuracy RS Oph’s behaviour in the coming weeks and months, owing to the masses of good data accrued over its previous outburst. RS Oph is likely to decline by 0.1 magnitude per day for the next 40 days or so, and then fade more slowly, by around 0.02 magnitude in the next 65 days, by which time it should be back to its pre-outburst brightness.

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Nova - RS Ophiuchi, Prabhakaran