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Archive for November, 2015

November 28, 2015

Ariane 5 VA227 Liftoff

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Arianespace dixit:

“Arianespace successfully launched two satellites [on November 10]: Arabsat-6B (BADR-7) for the operator Arabsat, and GSAT-15 for ISRO (Indian Space Research Organisation). The company’s tenth launch of the year from the Guiana Space Center (CSG), and sixth with the Ariane 5 heavy launcher, took place on November 10 at 6:34 pm local time in Kourou, French Guiana. Through this mission, the 69th successful launch in a row by Ariane 5, Arianespace is proud to deliver reliable, sustainable solutions to Arabsat and ISRO, two loyal customers for over 30 years.

Arabsat is the leading regional satellite telecommunications operator in the Middle East and Africa. Arabsat-6B (BADR 7) is the ninth satellite orbited by Arianespace for this operator since the launch of Arabsat-1A in 1985. This satellite is the first of the sixth generation of satellites in the Arabsat fleet. It will provide telecommunications and direct- to-home (DTH) TV broadcast services for the Middle East, Africa and Central Asia. In 2012 Arabsat also confirmed its goal of bolstering its position in the Europe-Middle East-Africa (EMEA) zone by acquiring the company Hellasat. Arianespace will be launching another Arabsat satellite, Hellasat-4.

GSAT-15 is the 19th satellite to be launched by Arianespace for ISRO (Indian Space Research Organisation). It will provide telecommunications services for the country, along with dedicated navigation-aid and emergency services. Arianespace has launched 91% of ISRO’s geostationary satellites that used non-Indian launch systems, dating back to the launch of the country’s experimental satellite APPLE on Flight L03 in 1981. The favored relationship between Arianespace and ISRO reflects the exemplary collaboration in the space sector between France and India, a partnership that will help ISRO realize its aim of using space to foster the development of the Indian sub-continent through a full range of satellite applications, for Earth observation, telecommunications, science and navigation.”

Video credit: ESA

 

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November 25, 2015

LISA Pathfinder

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Wikipedia dixit:

“LISA Pathfinder will place two test masses in a nearly perfect gravitational free-fall, and will control and measure their relative motion with unprecedented accuracy. The test masses and their environment will be the quietest place in the Solar System.

LISA Pathfinder is a proof-of-concept mission to prove that the two masses can fly through space, untouched but shielded by the spacecraft, and maintain their relative positions to the precision needed to realize a full-up gravitational wave observatory later. The primary objective is to measure deviations from geodesic motion. Much of the experimentation in gravitational physics requires measuring the relative acceleration between free-falling, geodesic reference test particles.

In LISA Pathfinder, precise inter-test-mass tracking by optical interferometry will allow scientists to assess the relative acceleration of the two test masses, situated about 38 cm apart in a single spacecraft. The science of LISA Pathfinder consists of measuring and creating an experimentally-anchored physical model for all the spurious effects – including stray forces and optical measurement limits – that limit the ability to create, and measure, the perfect constellation of free-falling test particles that would be ideal for the eLISA follow up mission. In particular, it will verify: drag-free attitude control of a spacecraft with two proof masses, the feasibility of laser interferometry in the desired frequency band (which is not possible on the surface of Earth), and the reliability and longevity of the various components—capacitive sensors, microthrusters, lasers, and optics.

For the follow-up mission, eLISA, the test masses will be 2 kg cubes housed in two separate spacecraft one million kilometers apart.”

Video credit: ESA

 

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November 18, 2015

Sentinel-2

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Wikipedia dixit:

“Sentinel-2 will serve a wide range of applications related to Earth’s land surface and coastal zones. The mission will mainly provide information for agricultural and forestry practices and for helping manage food security. Satellite images will be used to determine various plant indices such as leaf area chlorophyll and water content indexes. This is particularly important for effective yield prediction and applications related to Earth’s vegetation. As well as monitoring plant growth, Sentinel-2 can be used to map changes in land cover and to monitor the world’s forests. It will also provide information on pollution in lakes and coastal waters. Images of floods, volcanic eruptions and landslides contribute to disaster mapping and help humanitarian relief efforts.

Examples for applications include: monitoring land cover change for environmental monitoring; agricultural applications, such as crop monitoring and management to help food security; detailed vegetation and forest monitoring and parameter generation (e.g. leaf area index, chlorophyll concentration, carbon mass estimations); observation of coastal zones (marine environmental monitoring, coastal zone mapping); inland water monitoring; glacier monitoring, ice extent mapping, snow cover monitoring; flood mapping & management (risk analysis, loss assessment, disaster management during floods).”

Video credit: ESA

 

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November 7, 2015

Aurora Borealis

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ESA dixit:

“Still images taken by ESA astronaut Samantha Cristoforetti on the International Space Station were joined together to create this timelapse. The astronauts on the Space Station spend as much time as possible on science. During her 40-hour working week Samantha runs many experiments from Italy’s ASI space agency and ESA, and takes part in even more from scientists all over the world.”

Wikipedia dixit:

“An aurora is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions. Auroras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere), where their energy is lost. The resulting ionization and excitation of atmospheric constituents emits light of varying colour and complexity. The form of the aurora, occurring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating particles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton auroras are usually observed at lower latitudes.”

Video credit: ESA

 

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November 3, 2015

2015 TB145

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NASA JPL dixit:

“JPL scientist Marina Brozovic explains how radar will be used to study asteroid 2015 TB145 when it safely passes Earth on Oct. 31, 2015. Scientists are tracking the Halloween flyby with several optical observatories and the radar capabilities of the agency’s Deep Space Network at Goldstone, California. Radar images should be available within a few days of the flyby.
The asteroid will fly past Earth at a safe distance slightly farther than the moon’s orbit on Oct. 31 at 10:01 a.m. PDT (1:01 p.m. EDT). Scientists are treating the flyby of the estimated 1,300-foot-wide (400-meter) asteroid as a science target of opportunity.”

Video credit: NASA JPL

 

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