News roundup...
India’s heaviest communication satellite GSAT-11 launched successfully from French Guiana
Indian Space Research Organisation’s (ISRO) heaviest and most-advanced high throughput communication satellite GSAT-11 was successfully launched from the Spaceport in French Guiana during the early hours today.
GSAT-11 HTS (High-Throughput Satellite) in Clean Room prior to shipping to French Guiana. GSAT-11 reportedly has a throughput rate of 16 Gbps (which itself is a leap over the >1 Gbps data rates of non-HTS satellites), whereas future satellites from ISRO's HTS range will have speeds to the tune of ~100 Gbps.
The launch vehicle
Ariane 5 VA-246 lifted off from Kourou Launch Base, French Guiana at 02:07 am (IST) carrying India’s GSAT-11 and South Korea’s GEO-KOMPSAT-2A satellites, as scheduled. Ariane 5 is one of three launch vehicles operated by Arianespace along with Soyuz and Vega. After a 30-min flight, GSAT-11 separated from the Ariane 5 upper stage in an elliptical Geosynchronous Transfer Orbit. The achieved orbit was very close to the intended one.
The
5,854-kg GSAT-11 will provide high data rate connectivity to users of Indian mainland and islands through 32 user beams in Ku-band and 8 hub beams in Ka-band. “GSAT-11 will boost the broadband connectivity to rural and inaccessible Gram Panchayats in the country coming under the Bharat Net Project, which is part of Digital India Programme,” ISRO Chairman Dr K Sivan said.
The Bharat Net Project aims to enhance the public welfare schemes like e-banking, e-health, e-governance among others.
He said
GSAT-11 will act as a forerunner to all future high throughput communication satellites. “Today’s successful mission has boosted the confidence of the entire team,” Dr Sivan added. Post-separation, ISRO's Master Control Facility at Hassan in Karnataka took over the command and control of GSAT-11 and found its health parameters normal.
Ariane-5 VA-246 liftoff from Kourou, French Guiana, carrying the GSAT-11 as well as a South Korean satellite
The scientists will undertake phase-wise orbit-raising manoeuvres in the days ahead to place the satellite in the Geostationary Orbit (36,000 km above the equator) using its on-board propulsion systems. GSAT-11 will be positioned at 74-degree east longitude in the geostationary orbit.
Subsequently, the two solar arrays and four antenna reflectors of GSAT-11 will be deployed in orbit. The satellite will be operational after the successful completion of all in-orbit tests.
In the last 21 days, ISRO successfully completed three satellite and two launch vehicle missions.
India’s heaviest communication satellite GSAT-11 launched successfully from French Guiana - ISRO
UPDATE: As of today, all the Orbit-Raising Maneuvers on the GSAT-11 have been successfully performed by ISRO's Master Control Facility (MCF), Hassan.
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AstroSat Picture of the Month (APOM) Nov, 2018
Hot Ultraviolet stars in the Globular Cluster NGC 288
This month, APOM presents ultraviolet images of the
globular cluster NGC 288, located at a
distance of around 30,000 light years in the constellation Sculptor. This cluster was first described by
John Dreyer in 1888. This is the second globular cluster in the APOM series, the first one being
NGC 1851, presented a year ago. A
globular cluster is a very large group of stars formed from the same cloud of gas and dust at nearly the same time. They are called globular because of the spherical distribution of stars, and each cluster is held together as a single entity by the gravity of the star members. Globular clusters are few of the
oldest known objects in our galaxy. The stars in NGC 288 are believed to be nearly 12.6 billion years old.
The Ultraviolet Imaging Telescope (UVIT) on AstroSat has been used to image the stars in NGC 288 in the ultraviolet light, by a group of researchers from the Indian Institute of Astrophysics, Bangalore, and the National Research Council of Canada. The number of stars seen in the far-ultraviolet light are fewer than those seen in the near-ultraviolet light, and the reason for this is that only the hottest stars are seen in the far-ultraviolet.
Since globular clusters have very old stars, many of the heavier ones have already evolved to later phases of stellar lives (eg.
red giant stars,
horizontal branch stars). About 115 hot
horizontal branch stars having surface temperature nearly twice that of the surface of Sun have been detected in NGC 288 using the near and far-ultraviolet filters of UVIT. A couple of very hot stars (
extreme horizontal branch stars) whose whose surface temperatures are nearly five times that of the Solar surface have also been found. Using a combination of ultraviolet and optical light, these researchers have also identified 68 blue stragglers in this cluster. A
blue straggler is a star formed when two stars either
merge or transfer mass between them.
Such stars have been mostly found in globular clusters where the star density is high. The capabilities of UVIT have made it easy for the researchers to see and inspect hot stars towards the cluster individually, allowing them to study the properties of each star, such as the mass and temperature.
AstroSat Picture of the Month Nov, 2018 - ISRO
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HySIS First day Image
The 1st Day image from the Hyperspectral Imaging Satellite HysIS, was acquired at NRSC Hyderabad on 02 December 2018, covering parts of Lakhpat in Gujarat. The sample color composite image represents VNIR spectral bands.
Glimpse of HyperSpectral Data Captured by HySIS
Hyperspectral Cubes of different terrain conditions and sample spectral plots, depicting different features
Hi-res download:
Glimpse of HyperSpectral Data Captured by HySIS - ISRO