A
newly-discovered nova in Lupus is on the rise and approaching naked-eye visibility. Here's how to see it.

© Piqui DiazThe new nova in Lupus, formally named V462 Lupi, shines here at around magnitude 8.5 on June 15.2 UT. Photo taken through 8×42 binoculars with a smartphone. The nova's coordinates (J2000) are RA 15h 08m 03.3s, Dec. –40° 08″ 29.6′. North is up.
Exciting news! On June 12th (June 12.9 UT), the
All-Sky Automated Survey for Supernovae (ASAS-SN)
discovered a new 8.7-magnitude stellar object in Lupus. Not long after, Yusuke Tampo, with the South African Astronomical Observatory (University of Cape Town),
obtained a spectrum of the "new star" and identified it as a classical nova based on its spectral features and dramatic increase in brightness.
The nova went through a slew of temporary names — AT 2025nlr, ASASSN-25cm, and N Lup 2025 — until receiving its official designation V462 Lupi on June 16th. Since discovery, the nova has brightened rapidly. As of 8 p.m. Eastern Time June 16th, it's at magnitude 6.4 and flirting with naked-eye visibility. The magnitude rise has been phenomenal when you consider that prior to the explosion, the progenitor star was approximately magnitude 22.3 (in the blue band) according to American Association for Variable Stars (AAVSO) observer
Sebastián Otero, who dug up an older image from a photographic plate.

© Stellarium with additions by Bob KingThe new nova in Lupus is near a trio of naked-eye stars — Delta (δ) Beta (β) Lupi and Kappa (κ) Centauri. I've circled them here and on the more detailed AAVSO chart below.

© Courtesy of the AAVSO with additions by Bob KingUse this AAVSO chart to exactly locate the new nova as well as to estimate its brightness using the comparison stars provided. I've outlined a small triangle of 5th and 6th magnitude stars that will also be helpful in finding the nova. Stars are shown with decimals omitted; for example, 27 is magnitude 2.7.
Despite a southerly declination of -40°, the nova is bright enough to observe even in the northern United States. For instance, at my latitude 0f 47°N, the nova stands 3° above the horizon at meridian crossing. While that may sound hopeless, V462 Lupi will still shine around magnitude 9 after factoring in 2.5-magnitudes for extinction due to thick air in the horizon direction. Give me an unobstructed horizon, and I'll be ready to spring into action.

© ESO / M. KornmesserA nova always involves two closely-orbiting stars — a white dwarf and a companion star. In this artist view, the white dwarf (at left) robs gas from its companion (at right). The material forms an accretion disk around the dwarf before spiraling down to the surface, where it's heated and compressed until it ignites in a thermonuclear blast. The explosion causes the system to brighten by many millions of times — as much as 15 magnitudes!
If you're observing from a latitude around 40°N, the newcomer climbs to a comfortable 10° at meridian crossing, which occurs around 10:30 p.m. local time. From Tucson it reaches 18° altitude. You've got this! Nova explosions reaching 6th magnitude or brighter are uncommon, so treat yourself to a look the next clear night. The basic Stellarium map provided here should get you there. Then you can use the American Association of Variable Star Observers (AAVSO) map to pinpoint the nova's position and estimate its changing brightness in the nights ahead.
To keep up on its brightness changes, head over to the
AAVSO. Scroll up, type the name V462 Lup in the
Pick a Star box, and select the
Check Recent Observations link. You can also make additional charts as well as create a light curve for the nova at the site.
Happy hunting!
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