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Horie said his company's low-cost MOMO-3 rocket is the way to create a competitive space business in Japan. VOA

India is planning to launch its radar imaging satellite RISAT 2BR1 sometime towards the end of May 2019 on one of the variants of its Polar Satellite Launch Vehicle (PSLV) rocket, sources said on Tuesday.

The PSLV rocket is expected to fly on May 22 carrying RISAT 2BR1, officials of Indian Space Research Organisation (ISRO) told IANS on condition of anonymity.



The PSLV rocket is expected to fly on May 22 carrying RISAT 2BR1, officials of Indian Space Research Organisation (ISRO) told. Pixabay

The rocket that would carry RISAT 2BR1 is designated as PSLV-C46 as per ISRO’s numbering system and will blast off from the first launch pad at the country’s rocket port in Sriharikota.

ALSO READ: CMFRI, ISRO Join Hands to Protect Coastal Wetlands

Following the launch of RISAT 2BR1, ISRO will send up a cartography satellite Catosat-3. India will also launch two more defence satellites some time in July or August with its new rocket Small Satellite Launch Vehicle (SSLV). (IANS)


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Milky Way galaxy as seen from Chitkul Valley

NASA's Chandra X-ray Observatory has for the first time spotted signs of a planet transiting a star outside of the Milky Way galaxy, opening up a new avenue to search for exoplanets at greater distances than ever before.

The possible exoplanet -- or planets outside of our Solar System -- candidate is located in the spiral galaxy Messier 51 (M51), also called the Whirlpool Galaxy because of its distinctive profile, NASA said in a statement.

Astronomers have, so far, found all other known exoplanets and exoplanet candidates in the Milky Way galaxy, almost all of them less than about 3,000 light-years from Earth.

An exoplanet in M51 would be about 28 million light-years away, meaning it would be thousands of times farther away than those in the Milky Way, NASA said.

"We are trying to open up a whole new arena for finding other worlds by searching for planet candidates at X-ray wavelengths, a strategy that makes it possible to discover them in other galaxies," said Rosanne Di Stefano of the Center for Astrophysics at Harvard and Smithsonian (CfA) in Cambridge, Massachusetts, who led the study.

The findings are published in the journal Nature Astronomy.

The exoplanet candidate was spotted in a binary system called M51-ULS-1, located in M51. This binary system contains a black hole or neutron star orbiting a companion star with a mass about 20 times that of the Sun. The X-ray transit they found using Chandra data lasted about three hours, during which the X-ray emission decreased to zero.

Based on this and other information, the team estimates the exoplanet candidate in M51-ULS-1 would be roughly the size of Saturn and orbit the neutron star or black hole at about twice the distance of Saturn from the Sun.

The team looked for X-ray transits in three galaxies beyond the Milky Way galaxy, using both Chandra and the European Space Agency's XMM-Newton. Their search covered 55 systems in M51, 64 systems in Messier 101 (the "Pinwheel" galaxy), and 119 systems in Messier 104 (the "Sombrero" galaxy).

However, more data would be needed to verify the interpretation as an extragalactic exoplanet. One challenge is that the planet candidate's large orbit means it would not cross in front of its binary partner again for about 70 years, thwarting any attempts for a confirming observation for decades, NASA said.

Named in honor of the late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar, the Chandra X-ray Observatory is the world's most powerful X-ray telescope. It has eight times greater resolution and is able to detect sources more than 20-times fainter than any previous X-ray telescope.

Known to the world as Chandra (which means "moon" or "luminous" in Sanskrit), Chandrasekhar was widely regarded as one of the foremost astrophysicists of the twentieth century. (IANS/JB)


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