SN2014J – supernova in M82

M82 and SN2014J with D50 telescope.

Image of M82 and SN 2014J obtained with the D50 telescope on January 25th, 2014.

The nearest type Ia supernova in 400 years has been found in the Messier 82 (M82) galaxy. First spotted on 21 January 2014, it is relatively close to Earth, about 11.4 million light years away!
This supernova is called SN2014J (the 10th supernova discovered so far during 2014), and is a rare kind. “Type Ia” supernovae (SNe) are believed to be caused by exploding white dwarf stars. These SNe explode with very predictable brightnesses, making them ideal ‘standard candles’ to measure distances to galaxies accurately.

Now that it has reached maximum brightness, around Jan 31 (with a magnitude in the R band of about 10), GLORIA will keep monitoring the SN2014J light-curve (along with other supernovae) for the next few months as part of the regular program conducted by some of the GLORIA partners. Indeed, many astronomical observatories worldwide (including space-borne facilities) will point to this unique target regularly over the coming weeks.

M82 and SN2014J with D50 telescope.

Image of M82 and SN 2014J (M81 galaxy on the right) obtained with the BART telescope wide field camera on January 25th, 2014.

Gaia on its way to L2

ESA’s Gaia mission will create the most accurate map yet of the Milky Way. By making accurate measurements of the positions and motions of 1% of the total population of roughly 100 billion stars, it will answer questions about the origin and evolution of our home Galaxy. The Soyuz launcher, operated by Arianespace lifted off at 09:12 GMT on Dec 19 with Gaia on board. A few hours after, one of the GLORIA telescopes, the Pi-of-the-Sky-North experiment at the BOOTES-1 astronomical station at ESAt/INTA-CEDEA in Huelva (Spain), recorded the spacecraft on its route towards an orbit around a gravitationally-stable virtual point in space called L2, some 1.5 million kilometres from Earth in the direction opposite to the Sun.

For a full report on the launch from Michael Perryman go here.


Bird’s eye view of the Gaia launch

Michael Perryman was the scientific leader of ESA’s Hipparcos space astrometry mission, and with Lennart Lindegren from Sweden, one of the two originators of the Gaia mission. Michael is currently Bohdan Paczynski Visiting Fellow at the School of Astrophysical Sciences, Princeton and Adjunct Professor in the School of Physics, University College Dublin. Here he shares his ringside view of the launch.


19 December 2013: Today, at 06:12 local time here in French Guiana, the Gaia satellite was delivered into orbit, on its way to its surveying location, the Sun-Earth Lagrange point L2. So began the latest and most revolutionary journey in the history of the measurement of the positions of the stars. Placed in orbit by the 1812th launch of the vast Russian Soyuz programme (their 6th from French Guiana), Gaia marks the 40th launch for ESA, and the 25th scientific satellite lofted by Arianespace. To wish it well on its historic journey were a representation of Gaia scientists, ESA project managers and engineers headed by ESA’s Director of Science Alvaro Gimenez, industrial leaders, national delegates to ESA, and senior representatives from numerous other fields of the increasingly ambitious European space programme.

Gaia first appeared as a proposal for consideration in ESA’s space programme in 1993, hot on the heels of ESA’s revolutionary Hipparcos star-mapping mission launched in 1989. Seven years of careful study led to its acceptance by ESA’s Science Programme Committee in 2000, with a target launch date of 2012. Maintaining such an aggressive schedule, for such an ambitious mission at the forefront of so many areas of space technology, is almost unheard of. Managed by ESA, with manufacture, integration and testing contracted to the mission’s prime contractor, Astrium Toulouse, the Gaia industrial consortium comprised 47 European and three US industrial partners. It will map the stars at unprecedented and almost incomprehensible levels of accuracy. The largest instrument built in silicon carbide, Gaia also comprises the largest billion-pixel CCD focal plane ever conceived.

Shipped out from Europe in August, the launch countdown started at t-11 hours. At t-30 min, all systems were go, and weather conditions were perfect. As dawn broke over the Atlantic coast of French Guiana, just outside Kourou, the final 10 second countdown began. Silence fell over the assembled spectators as lights began to flicker amongst the trees on the horizon, then the sky lit up, the ground rumbled beneath us, and the colossal Soyuz powered into the sky. Hidden for a few moments by a thin layer of cloud, Soyuz appeared majestically seconds later, carrying its celestial surveyor in an awesome display of terrifying power. At 170km altitude the upper stage continued to carry Gaia almost vertically upwards. At 38 min after lift-off, no longer visible but with its tell-tale vapour trail streaked across the sky, the launcher orientated the satellite in the direction of L2, before successfully releasing Gaia, now racing away from Earth. Already under the control of ESA’s space operations centre ESOC, in Germany, and just 77 minutes after launch, the next most critical phase of the satellite’s pioneering odyssey, was successfully executed – the deployment of the colossal 10m diameter solar array and sunshield.

It was a perfect injection into the transfer to L2. It will still be a 20-day journey to the isolated expanse of L2, where Gaia will be ‘parked’. From that location, a lengthy process of payload commissioning will precede the 5-year operational phase. Gaia’s goal: to revolutionise the understanding of our Galaxy, and the stars within it.

The most crucial and spectacular step in the execution of all space missions has been passed. After more than a decade of intense dedication, colossal effort, and vast ingenuity, the make-or-break moment of every space mission was decided, in Gaia’s favour, within just a few short minutes. As Arianespace Chairman and CEO, Stéphane Israel, described it “Gaia is a technological marvel, which should make Europe proud of its space industry”.

Comet ISON flies too close to the Sun

Comet ISON at seen by the SOHO satellite on November 29th at 6.30 UT. Credits:

Is this the end of comet ISON?

Comet ISON has failed to survive its perihelion intact? Yes, but something is still there.
A few signs of unhealthy behaviour were observed in the days before it made its closest approach to the Sun. Being so close to the Sun must have been very “stressful” and what is left (see image) could disappear to our eyes very soon. For the time being, let’s keep watching.

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News from comet ISON

Comet C2012/S1 ISON: the brightest comet in the XXI century (so far) followed by GLORIA.

Comet ISON at dawn on November 21st (6:20 UT). The image was taken from the Teide Observatory (Instituto de Astrofísica de Canarias) with a digital camera (Canon 5D-MII, 85mm lens) and an exposure time of about 6 seconds. The brightest object in the image is the planet Mercury, while at the bottom center, just above the sea of ​​clouds, the peaks of the Gran Canaria island are visible. Credits: J.C. Casado,

On its way to the Sun, comet C2012/S1 ISON will continue to brighten, but it will also get harder and harder to see since it will be close to the Sun in the sky. Right now the comet is close to the eastern horizon before dawn. See the 3-D model.

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View the timelapse from the Teide observatory on YouTube:
November 21st, 2013
November 22nd, 2013

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