पीड़ितों को मिले न्याय, समय से वितरण करे राहत एवं आर्थिक सहायता- सीडीओ

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देहरादून: मुख्य विकास अधिकारी अभिनव शाह की अध्यक्षता में शुक्रवार को विकास भवन में अनुसूचित जाति, जनजाति (अत्याचार निवारण) अधिनियम-1995 के अंतर्गत गठित जिला स्तरीय सतर्कता एवं अनुश्रवण समिति की बैठक हुई। बैठक में अधिनियम के अंतर्गत वर्ष 2021 से अभी तक पीड़ितों के प्राप्त प्रकरणों और उनको राहत व आर्थिक सहायता वितरण कार्यो की विस्तृत समीक्षा की गई।

मुख्य विकास अधिकारी ने निर्देश दिए कि अधिनियम के अंतर्गत लंबित प्रकरणों का जल्द से जल्द निस्तारण करते हुए पीड़ितों को राहत प्रदान की जाए। सीडीओ ने पुलिस विभाग को निर्देशित किया कि विगत पांच वर्षो में अधिनियम के अंतर्गत पंजीकृत प्रत्येक प्रकरण की अद्यतन सूचना 15 दिनों के भीतर उपलब्ध करें। समाज कल्याण विभाग को रोस्टर निर्धारित करते हुए हर तीन माह में समिति की बैठक रखने के निर्देश दिए। ताकि लंबित प्रकरणों का त्वरित समाधान हो सके और पीड़ितों को समय पर न्याय और राहत मिल सके।

इस दौरान बताया गया कि अनुसूचित जाति, जनजाति अत्याचार निवारण अधिनियम के अंतर्गत वर्ष 2021 से 2025 तक जनपद में मारपीट, गाली गलौज, जाति सूचक शब्द के 47 मामले, छेडछाड, लज्जा भंग के 07, बलात्कार के 08, हत्या का 01 सहित कुल 63 प्रकरण पंजीकृत हुए है, जिनमें से कुछ प्रकरणों का निस्तारण कर लिया गया है जबकि अवशेष प्रकरणों पर सुनवाई चल रही है। मारपीट, गाली गलौज, जातिसूचक शब्द के कुछ प्रकरणों के निस्तारण के तहत वर्ष 2021 से अब तक रु0 32.18 लाख की राहत एवं आर्थिक सहायता का वितरण किया गया है। वहीं छेडछाड, लज्जा भंग में 09 लाख, बलात्कार के मामले में 24 लाख, हत्या के मामले में 8.25 लाख की धनराशि पीड़ितों को आर्थिक सहायता के रूप में वितरित की जा चुकी है।

बैठक में मा0 विधायक रायपुर उमेश शर्मा काऊ, मा0 विधायक खजान दास के प्रतिनिधि गोपाल पुरी, समिति के सदस्य सतीश कुमार, जनक सिंह, परियोजना निदेशक डीआरडीए विक्रम सिंह, जिला समाज कल्याण अधिकारी दीपांकर घिल्डियाल, निरीक्षक पुलिस विभाग केआर पांडेय, डीपीओ जितेंद्र कुमार आदि उपस्थित थे।

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  51. A star with a larger mass burns more quickly and intensely
    than a smaller-mass star due to larger stars needing to burn more fuel to
    prevent its collapse. The specific causes of
    these winds remain unknown, but if they generally accompany
    star formation, astronomers will have to consider the
    implications for the early solar system. The remnant of a supernova observed in 1572, notably studied by the Danish astronomer Tycho Brahe, lies about 13,000 light-years away in the
    constellation Cassiopeia. All that’s left of the star
    is its core, now called a white dwarf, a roughly
    Earth-sized stellar cinder that gradually cools over billions of
    years. More massive stars must burn fuel at a higher rate to generate the energy that keeps them from
    collapsing under their own weight. In more massive stars, helium is produced in a cycle of
    reactions catalyzed by carbon called the carbon-nitrogen-oxygen cycle.

    Positioned at the heart of the multi-billion-dollar Queen’s Wharf Brisbane precinct,
    The Star Brisbane commenced its staged opening IN August 2024 – redefining Brisbane’s riverfront as
    a world-class tourism, entertainment and lifestyle destination. With a radius
    of nearly 1.5 billion kilometers (930 million miles),
    it is 2,150 times wider than the Sun. Stephenson 2-18 is
    the largest star that astronomers have recorded in the universe.
    Because of this energy cycling, astronomers believe that some low-mass dwarfs can last up to 14 trillion years.
    The dense remnants of the star’s core after the supernova
    are known as neutron stars. Once a star is in the white dwarf stage, it only cools and no
    longer produces new heat.
    This process provides the energy that fuels the star and prevents it from collapsing under the force of gravity.
    Proxima Centauri is a red dwarf star, roughly seven times smaller than our Sun and only about 50% larger than Jupiter.
    However, once silicon in the star fuses into iron, it will abruptly run out of fuel within merely a few days.
    These new elements become the star’s fuel, which prevents
    the star from collapsing for longer. The white dwarf that remains will begin to cool over the course of billions of
    years.
    A number of private companies sell names of stars which are not recognized by the IAU,
    professional astronomers, or the amateur astronomy community.
    (Uranus and Neptune were Greek and Roman gods, but neither planet was known in Antiquity because of their low
    brightness. Their names were assigned by later astronomers.) With
    the aid of gravitational lensing, a single star
    (named Icarus) has been observed at 9 billion light-years away.
    Individual stars such as Cepheid variables have been observed in the M87 and
    M100 galaxies of the Virgo Cluster, as well as luminous stars in some other relatively nearby
    galaxies.
    Fusion converts carbon into heavier elements like oxygen, neon, and magnesium, which will
    become future fuel for the core. Eventually, all the star’s outer layers blow away, creating an expanding cloud of dust and gas called a planetary nebula.
    The energy produced by fusion creates pressure inside the star that balances
    gravity’s tendency to pull matter together,
    so the core starts to collapse. Some low-mass stars will shine for trillions of years – longer than the universe has currently existed – while
    some massive stars will live for only a few million years.
    After millions of years, immense pressures and temperatures in the star’s core squeeze the nuclei of hydrogen atoms together to form helium, a process called nuclear fusion.
    The most massive stars last an average of a few million years,
    while stars of minimum mass (red dwarfs) burn their fuel very slowly and can last
    tens to hundreds of billions of years. When they occur within the Milky Way, supernovae have historically
    been observed by naked-eye observers as “new stars” where none seemingly existed before.
    The shockwave formed by this sudden collapse causes the rest of the star to explode in a supernova.
    Some massive stars, particularly luminous blue variables, are very unstable
    to the extent that they violently shed their mass into space in events known as supernova impostors, becoming significantly brighter in the process.

    Using the stellar spectrum, astronomers can determine the
    surface temperature, surface gravity, metallicity and rotational velocity of a star.
    Giant stars have much lower surface gravity than do main-sequence stars, while the opposite is the case for degenerate,
    compact stars such as white dwarfs. Smaller bodies called brown dwarfs, occupy a poorly defined grey area between stars
    and gas giants. Stars have masses ranging from less than half the solar
    mass to over 200 solar masses (see List of most massive stars).
    During the Maunder Minimum, for example, the Sun underwent
    a 70-year period with almost no sunspot activity.
    In massive stars, heavier elements can be burned in a
    contracting core through the neon-burning process and oxygen-burning process.
    For the Sun, the influence of its solar wind
    extends throughout a bubble-shaped region called the heliosphere.
    It is within the photosphere that sun spots, regions of lower than average temperature,
    appear. Stars with several times the mass of the Sun have a
    convection zone deep within the interior and a radiative zone in the outer
    layers. The resulting temperature and pressure at the hydrogen-burning core of a main-sequence star are sufficient
    for nuclear fusion to occur and for sufficient energy to be produced to prevent further collapse of the star.
    The explosion is created when the white dwarf accretes hydrogen from the companion star, building up mass until the hydrogen undergoes
    fusion. These range from 0 (hypergiants) through III (giants) to V (main-sequence dwarfs); some authors add VII
    (white dwarfs).
    Stellar mass loss or supernova explosions return chemically enriched
    material to the interstellar medium. A star’s life begins
    with the gravitational collapse of a gaseous nebula of material largely
    comprising hydrogen, helium, and traces of heavier elements.

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