Highlights

Radioastronomy at the speed of light

INAF’s radiotelescope at Noto, near Siracusa, plays a crucial role in European radioastronomy with its 32-meter dish, being one of the most southerly antennas in the European region. Since May 15, it is part of the international e-VLBI network. The VLBI (Very Long Baseline Interferometry).

Dual Site for SKA

The Members of the SKA Organisation agreed on a dual site solution for the Square Kilometre Array telescope, a crucial step towards building the world’s largest and most sensitive radio telescope. The ASKAP and MeerKAT precursor dishes will be incorporated into Phase I of the SKA which will deliver more science and will maximise on investments already made by both Australia and South Africa

Open position: Chief Communications officer for the SKA

The SKA Organisation announces the vacancy for the position of Chief Communications Officer.Closing date: 8 June 2012.

Vesta shown by NASA's Dawn mission

NASA's Dawn mission has rivealed new images of the giant asteroid Vesta, uncovering new intriguing secrects of its surface. The latest results include stunning colorized images that suggest that the giant asteroid has an unexpectedly wide variety of rocks on its surface and gravity data that show Vesta is curiously dense at the south pole.

Two oldest planets found: 12.8 billion years old

Four Italian astronomers have found the two oldest alien planets yet discovered. The two huge planets have been found orbiting a star 375 light-years away from the Earth and scientists estimate an age around 12,8 billion years.

EXOMARS: Esa goes on with Russian support

After NASA abandoned the EXOMARS project, the European Space Agency (ESA) turned to the support of the Russian Federal Space Agency (RosCosmos), which will donate the delivery system, the Proton rocket. The european mission will start in 2016. The comment of the President of INAF and COSPAR Giovanni Bignami.

The Italian Pathway to SKA

First National Meeting on Science and Technology with SKA MIUR - Rome, 19-20 giugno 2012

The engine of the Crab Nebula

The pulsar at the heart of the Crab nebula is bursting with energy. This was just confirmed by the MAGIC collaboration operating two large telescopes on the Canary islands. MAGIC observed the pulsar and found out periodic emission of short pulses stretching till the energies as high as 400 GeV. This is 50-100 times more than expected from theory.

Catania observatory meets prisoners

The astronomers of the Inaf, National institute for astrophysics, and the astronomical observatory of Catania have joined a new project called “L'Astronomia nei luoghi di disagio” (Astronomy in place of discomfort). Physicists and astronomers will teach to prisoners the life of the stars and some fundamentals of astronomy.

The Feeding Habits of Teenage Galaxies

New observations made with ESO’s Very Large Telescope are making a major contribution to understanding the growth of adolescent galaxies. In the biggest survey of its kind astronomers have found that galaxies changed their eating habits during their teenage years - the period from about 3 to 5 billion years after the Big Bang.

Solar Storm and auroras in progress

NASA claimed the second strongest solar storm just happened since the beginning of the new solar cycle. The comments of INAF’s solar astrophysicists Alessandro Bemporad and Mauro Messerotti.

The Hercules fighting galaxies

A new spectacular image from the VST (VLT Survey Telescope) the Italian instrument realized from INAF - OA Capodimonte in collaboration with ESO.

Re-Ionization: When and How?

National Workshop. April 11-12, 2012. IASF Milano, via Bassini 15, 20133 Milano

X-ray Astronomy: towards the next 50 years!

International conference, Oct 1st to Oct 5th, 2012, Milan (Italy)

The Time Machine Factory

We are pleased to announce that the conference "The Time Machine Factory" will be held in Torino (Italy), from October 14 to 19, 2012. The conference is being organized by Osservatorio Astrofisico of Torino- INAF, INRiM and Politecnico di Torino.

Highlights news

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