T. Puckett, Ellijay, GA, U.S.A.; Caroline Moore, Warwick, NY, U.S.A.; and Jack
Newton, Portal, AZ, U.S.A., report the discovery of an apparent supernova
(mag 18.8) on unfiltered CCD images (limiting mag 19.4) taken with a 0.40-m
reflector at Portal on Nov. 7.17 UT in the course of the Puckett Observatory
Supernova Search. The new object was confirmed at mag 18.2 on images
(limiting mag 19.8) taken by Ton Orff on Nov. 9.16 with a 0.60-m reflector at
Ellijay. SN 2008ha is located at R.A. = 23h34m52s.69, Decl. = +18o13'35".4
(equinox 2000.0), which is about 12" west and 0".5 south of the center of
UGC 12682. Nothing is visible at this position on images taken by Puckett
on Sept. 8 (limiting mag 19.4). The exact center of the apparent host
galaxy was very hard to measure, so its coordinates were taken from the
Sinbad website (position end figures 53s.55, 35".9), though Puckett's
measurements on the brightest nodule yield position end figures 53s.31, 38".0.


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.

(C) Copyright 2008 CBAT
2008 November 10 (CBET 1567) Daniel W. E. Green

Surrounded by three of her telescopes in a shed-style observatory,
14-year-old Caroline Moore is the youngest person ever
to discover an extragalactic supernova. Photo courtesy of Robert Moore

.......................................................................................................

Here are some photos:





Warwick Town Board Supervisor Michael Sweeton presents Caroline with her certificate.




Supervisor Sweeton looks over some images of Caroline's supernova

Peculiar Small Supernova Discovered By New York Teen

In November 2008, Caroline Moore, a 14-year-old student from upstate New York, discovered a supernova in a nearby galaxy, making her the youngest person ever to do so. Additional observations determined that the object, called SN 2008ha, is a new type of stellar explosion, 1000 times more powerful than a nova but 1000 times less powerful than a supernova. Astronomers say that it may be the weakest supernova ever seen. Even though this explosion was a weakling compared to most supernovae, for a short time SN 2008ha was 25 million times brighter than the sun. However, since it is 70 million light years away, it appeared very faint viewed from Earth. The peculiar object effectively bridged the gap between a nova (a nuclear explosion on the surface of an old, compact star called a white dwarf) and a type Ia supernova (the destructive death of a white dwarf caused by a runaway nuclear reaction starting deep in the star). SN 2008ha likely was a failed supernova where the explosion was unable to destroy the entire star. "If a normal supernova is a nuclear bomb, then SN 2008ha is a bunker buster," said team leader Ryan Foley, Clay fellow at the Harvard-Smithsonian Center for Astrophysics and first author on the paper reporting the findings. "From one perspective, this supernova was an underachiever, however you still wouldn't want be anywhere near the star when it exploded." Caroline was able to discover the object using a relatively small telescope, but some of the most advanced telescopes in the world were needed to determine the nature of the explosion. Data came from the Magellan telescopes in Chile, the MMT telescope in Arizona, the Gemini and Keck telescopes in Hawaii, and NASA's Swift satellite. In typical supernova explosions, light from different chemical elements (such as calcium or iron) is smeared out across the electromagnetic spectrum by the Doppler effect (the same principle that makes a police siren change pitch as it passes). Because the ejected bits of the star were "only" moving at 4.5 million miles per hour (compared to 22 million miles per hour for a typical supernova), the light wasn't as smeared out, allowing the team to analyze the composition of the explosion to a new precision. "You can imagine many ways for a star to explode that might resemble SN 2008ha," said Robert Kirshner of the Harvard-Smithsonian Center for Astrophysics. "It could have been a massive star suddenly collapsing to form a black hole, with very little energy leaking out. But it looks a lot like its brighter cousins, which we think are nuclear explosion of white dwarfs. Maybe this one was an explosion of that general type, just much, much weaker." One reason astronomers haven't seen this type of explosion before might be because they are so faint. "SN 2008ha was a really wimpy explosion," said Alex Filippenko, leader of the University of California, Berkeley supernova group, which monitors thousands of relatively nearby galaxies with a robotic telescope at Lick Observatory in California. But a new generation of telescopes and instruments is beginning to search greater distances than ever before, effectively monitoring millions of galaxies. Foley's team concludes that hundreds of this type of event may be spotted in the next few years. "Coincidentally, the youngest person to ever discover a supernova found one of the most peculiar and interesting supernovae ever," remarked Filippenko. "This shows that no matter what your age, anyone can make a significant contribution to our understanding of the Universe."
related report


Queen Astronomers Propose New Supernova Interpretation
Belfast, UK (SPX) Jun 12, 2009 - In a controversial new paper in the journal Nature, astronomers from Queen's University Belfast have proposed a new physical interpretation of a supernova discovered on 7th November 2008. A group of researchers, led by Dr. Stefano Valenti from Queen's University Belfast, found a weak explosion that is unusual in many ways, and several lines of evidence suggest it could be from a massive star. This goes against mainstream thinking in the astrophysics community which believes that this type of supernova comes from old white dwarf stars (low-mass stars) in binary systems.
The supernova in question SN2008ha was a faint explosion that contained no hydrogen. In their paper however, Valenti and his colleagues propose that the peculiar spectrum and faint luminosity of the supernovae in question, SN2008ha, more closely resembles those supernovae associated with the death of massive stars when their core collapses. The key difference with the other faint explosion of massive stars was the lack of hydrogen which is usually detected in underluminous Supernovae. Dr Valenti said "SN2008ha is the most extreme example of a group of supernovae that show similar properties. Up until now the community had thought that they were from the explosion of white dwarfs, which we call type Ia supernovae. Those are the ones that have been used to measure the geometry of the distant Universe and infer the existence of dark energy. But we think SN2008ha doesn't quite fit this picture and appears physically related to massive stars" Professor Stephen Smartt from Queen's added "This is still quite controversial, we have put this idea forward and it certainly needs to be taken seriously. "The implications are quite important. If this is a massive star explosion then it is the first one that might fit the theoretical models of massive stars that lose their outer layers through their huge luminosity pressure and then, perhaps, collapse to black holes with a whimper". Dr Valenti's team is keen to use new deep, time resolved surveys of the Universe to find more of these and test their ideas. One such experiment is the first of the Pan-STARRS telescopes that has started surveying the sky in the last month. The supernova in question was found in the galaxy UGC12682 in the constellation Pegasus by American school girl Caroline Moore, a member of the Puckett Observatory Supernova Search team.
It was immediately recognized by professional astronomers as quite unique, as it was one of the faintest explosions of its type ever discovered, with an energy approximately 50 times smaller than usual. This is the equivalent of converting several earth masses completely into energy.

We present ultraviolet, optical, and near-infrared photometry as well as optical spectra of the peculiar supernova (SN) 2008ha. SN 2008ha had a very low peak luminosity, reaching only M_V = -14.2 mag, and low line velocities of only ~2000 km/s near maximum brightness, indicating a very small kinetic energy per unit mass of ejecta. Spectroscopically, SN 2008ha is a member of the SN 2002cx-like class of SNe, a peculiar subclass of SNe Ia; however, SN 2008ha is the most extreme member, being significantly fainter and having lower line velocities than the typical member, which is already ~2 mag fainter and has line velocities ~5000 km/s smaller (near maximum brightness) than a normal SN Ia. SN 2008ha had a remarkably short rise time of only ~10 days, significantly shorter than either SN 2002cx-like objects (~15 days) or normal SNe Ia (~19.5 days). The bolometric light curve of SN 2008ha indicates that SN 2008ha peaked at L_peak = (9.5 +/- 1.4) x 10^40 ergs/s, making SN 2008ha perhaps the least luminous SN ever observed. From its peak luminosity and rise time, we infer that SN 2008ha generated (3.0 +/- 0.9) x 10^-3 M_sun of 56Ni, had a kinetic energy of ~2 x 10^48 ergs, and ejected 0.15 M_sun of material. We classify three new (and one potential) members of the SN 2002cx-like class, expanding the sample to 14 (and one potential) members. The host-galaxy morphology distribution of the class is consistent with that of SNe Ia, Ib, Ic, and II. Several models for generating low-luminosity SNe can explain the observations of SN 2008ha; however, if a single model is to describe all SN 2002cx-like objects, either electron capture in Ne-Mg white dwarfs causing a core collapse, or deflagration of C-O white dwarfs with SN 2008ha being a partial deflagration and not unbinding the progenitor star, are preferred. Abridged.