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All active supernova over mag 17.0
NameMagTypeHost
2024qvh14.4IIESO 138-G14
2024pxg14.7*IINGC 6221
2024phv14.8*IINGC 3936
2024jlf14.9IINGC 5690
2024ggi15.3*IINGC 3621
2024vcs15.9IIanonymous
AT2024vmx16.0unknone
AT2024uai16.0Ia-91bgNGC 2300
AT2024qev16.1*unknone
ASASSN-24dx16.1IIUGC 1118
2024ufz16.2IaESO 387-G29
2024qiw16.2*IILEDA 16241
AT2024qbs16.3*unknone
2024sky16.3IINGC 6492
2024sfk16.3IaAGC 111938
2024pgy16.3*IaUGC 11499
AT2024ubz16.4unknone
AT2024sjh16.5*unknone
AT2024rlc16.5unkIC 4350
AT2024psp16.5*unknone
2024pmm16.5*Ianone
AT2024sdj16.6*unknone
AT2024rrb16.6*unknone
2024qrp16.6*IILEDA 3213185
AT2024vau16.7unknone
ASASSN-24fn16.7unkESO 405-G15
2024sht16.7IaUGC 1347
2024nwu16.7*Iaanonymous
AT2024vhd16.8unknone
AT2024ugc16.8unknone
AT2024slr16.8unknone
AT2024svc16.9unkNGC 1671
AT2024sug16.9unkNGC 7476
2024uwq16.9Ic-BLNGC 6902
2024ttn16.9IaLEDA 2065235
2024slm16.9IaUGC 10246

* - last observation is over one month old.  

A long time ago, in a galaxy far far away, a star exploded.   This star exploded so violently that for a few weeks the star outshone its parent galaxy.   This type of explosion is called a Supernova.   The last one in our galaxy was 400 years ago, making us about 300 years overdue for the next one.   Here you will find a list of the supernovae we can see right now, as well as information about where they are in the sky, images of that object and how bright the explosion was at the last time we measured it.   The data on this page comes from TNS and ATEL circulars.   These web pages have brought you the latest in supernovae data and images since April 1997.   27 years and counting.

.   For yesterday's updates, go to the updates page.

News: Some of our brighter supernova are entering solar conjunction.   2024muv is just south of the core of NGC 4699.   2024iss is a bright supernova in a little galaxy in the Coma cluster.   2024inv is beginning to fade in NGC 3524.   2024ggi is a type II in the southern NGC 3621.   AT2016blu in NGC 4559 is back at mag 16.   You will notice that the magnitudes of the brighter objects (< 17.0) are now updated more often.   For the year 2024, 15346 supernovae (1320 CBAT, 14024 unconfirmed, and 2 other sources) have been reported. (20575 last year).   The brightest SN of the year 2024 are 2024ggi (Mag 11.7), followed by 2024inv (Mag 12.1), 2024muv (Mag 12.7), 2024any (Mag 12.7), 2024gy (Mag 12.8).  

The page now detects if you have set Dark Mode on your browser, please tell me if the colors don't work for you.   New User's manual.   New version of the web page for cell phone users: https://www.RochesterAstronomy.org/snimages/sn.html.   TNS has moved to a new URL: https://www.wis-tns.org/.   To post your discoveries, go to the TNS getting started page.   The Open supernova Catalog has died, links will be removed eventually.   Latest Supernovae is now supported by Purdue University and maintains a new mirror hosted in the Department of Physics and Astronomy that is overseen by Dan Milisavljevic.   Purdue mirror page: http://www.physics.purdue.edu/brightsupernovae/.   New features: Modifed the sorted by name list to include removed objects and mark "non public" objects. All galactic objects (CV novae, etc) will be banished on a weekly basis to the boneyard.   Thanks for all of the images, I have been posting them on flickr.   Join the discussion! Facebook Supernova Enthusiasts Group.   The Active supernovae page is a version of this page which is designed to be easier to read.   I've done extensive work recently in the Archives.   If anybody knows who some of the "unknown" discoverers are, please let me know.   Does anybody know of a grant that I could apply to for supporting this page? I probably spend about 2 hours a night working on it.   To turn off the icons, use this link.   With the demise of of Yahoo Groups, I am moving isn_chat to Google groups.   Please sign up if interested.  

2024vfo (= GOTO24fwv) (= ZTF24abhbrcs), TNS discovered 2024/09/11.582 by Koichi Itagaki
Found in UGC 690 at R.A. = 01h07m27s.385, Decl. = +39°24'13".60
Located 62".7 west and 11".9 north of the center of UGC 690 (Discovery image (mirror)) (Oyvind Kristiansen image)
Mag 18.5:9/12, Type II (zhost=0.019577) (References: ZTF observations)

AT2024unf, TNS discovered 2024/09/04.049 by Mascola
Found in NGC 3073 at R.A. = 10h00m50s.000, Decl. = +55°36'55".00
Located 17".6 west and 12".8 south of the center of NGC 3073
Mag 15.0:9/4, Type unconfirmed (zhost=0.003763)