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3rd International Conference on Astronomy, Astrophysics and Space Science, will be organized around the theme “”

Astro Physics 2020 is comprised of 21 tracks and 105 sessions designed to offer comprehensive sessions that address current issues in Astro Physics 2020.

Submit your abstract to any of the mentioned tracks. All related abstracts are accepted.

Register now for the conference by choosing an appropriate package suitable to you.

An exoplanet or extrasolar planet is a planet outdoor the Solar System. Exoplanets are very firm to see directly with telescopes. They are hidden by the cheerful stare of the stars they orbit. So, astronomers use other ways to notice and study these distant planets.

planetary physics (astrophysics) is the study of the structure, arrangement, and physical and chemical possessions of the planets of the solar system, counting their atmospheres and immediate cosmic environment.

 

  • Track 1-1Planetary science
  • Track 1-2 planetology
  • Track 1-3 planetary systems

The outside atmospheres of luminous cool huge stars and early type stars can be driven outward by radiation coming from the photosphere of the star. The radiation pressure forces the ounces outward, dragging ions along by viscous drag if the atmosphere is dense, thus creating a dust-driven wind.

 

  • Track 2-1stellar wind bubbles
  • Track 2-2Cosmic wind

supernova   is a powerful and luminous stellar explosion. A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova. The supernova remnant is bounded by an expanding shock wave, and consists of ejected material expanding from the explosion, and the interstellar material it sweeps up and shocks along the way. A planetary nebula, abbreviated as PN is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives.

 

  • Track 3-1Cosmic rays
  • Track 3-2pulsar wind nebula
  • Track 3-3Hypernova remnants

Brown dwarfs are substances which are too big to be called planets and too minor to be stars. They have crowds that range between twice the mass of Jupiter and the lower mass limit for nuclear reactions. An ultra-cool dwarf is a stellar or sub-stellar object of spectral class M that has an effective temperature under 2,700 K. TRAPPIST-1 is a widely known example of an ultra-cool dwarf star. Stars are enormous celestial bodies made mostly of hydrogen and helium that produce light and heat from the mixing nuclear forges inside their cores. Aside from our sun, the dots of bright we see in the sky are all light-years from Earth.

 

  • Track 4-1Deuterium fusion
  • Track 4-2Sub-brown dwarf

Atmospheric Sciences in the Department of Earth and Environmental Sciences comprise study of the movement, arrangement, and physical and chemical processes of the atmosphere. Timescales studied range from hours to millennia. Studies include the important processes of the atmosphere as well as its interactions with the oceans, hydrological cycle, cryosphere and biosphere, and the part of the atmosphere in anthropogenic climate alteration.

  • Track 5-1Meteorology
  • Track 5-2Climate Science
  • Track 5-3Oceanography
  • Track 5-4Geologic Hazards
  • Track 5-5Exploration Geophysics

The best-supported theory of our universe's source centers on an event known as the big bang. This theory was instinctive of the observation that other galaxies are stirring away from our own at great speed in all directions, as if they had all been pushed by an ancient explosive forc

  • Track 6-1Milky Way
  • Track 6-2Shell galaxy

All of the planets in our solar system orbit nearby the Sun. Planets that orbit around other stars are called exoplanets. All of the earths in our solar system orbit around the Sun. Planets that orbit around other stars are named exoplanets.

  • Track 7-1Planetary Astronomy
  • Track 7-2Heliocentrism
  • Track 7-3Speculation on Extrasolar Planetary Systems

Astronomical Computing and Applications is a peer-reviewed scientific journal cover research on applications computer science in astronomy published by Elsevier. It was established in 2013 and is inattentive and indexed in the Astrophysics Data System, INSPEC and Scopus.

  • Track 8-1Astronomical Data Analysis Software & Systems

Optical astronomy explanations using telescopes and recording media that imprisonment visible light. Optoelectronics is the study and submission of electronic devices and systems that source detect and control light, typically considered a sub-field of photonics.

  • Track 9-1Photoelectric effect
  • Track 9-2 photovoltaic effect
  • Track 9-3Photodiodes
  • Track 9-4Phototransistors
  • Track 9-5Photomultipliers
  • Track 9-6Optoisolators

Dark Matter is the slight portion of that visible matter current in the universe which sums up to form a total of 27 %. The matter is made up of particles called baryons. Scientists even though it’s a result of a long-discarded form of Einstein's theory of gravity, one that limited the "cosmological constant" but even that didn't give them the answer they were looking for. So they obviously take to name it is Dark Energy.  Almost 68% of the entire cosmos is dark energy, 27% composes of Dark Matter and all the other normal matter encompasses to 5%. Black Holes are great amount of matter packed together in a very small area which then results in huge gravitational force that even light could discharge through it.

 

  • Track 10-1Baryonic matter
  • Track 10-2Non-baryonic matter
  • Track 10-3Cold dark matter
  • Track 10-4Warm dark matter
  • Track 10-5Hot dark matter

The Planetary Society's dream is to know the cosmos and our place within it. Some space mission presented us just how far the human race can go, while others made us feel the depths of our grief. The crews and crafts complicated in these remarkable space missions made great paces in exploring our universe, and they will not soon be elapsed.

A satellite is a thing in space that orbits or loops around a superior object. Such as the International Space Station circling the Earth.

 

  • Track 11-1Flyby Space Missions
  • Track 11-2Orbiter Spacecraft
  • Track 11-3Rovers
  • Track 11-4Natural satellites
  • Track 11-5Artificial satellites

The cosmic microwave background (CMB, CMBR), in Big Bang cosmology, is electromagnetic radiation as a remnant from an early stage of the universe, also known as "artefact radiation". The CMB is pale cosmic background radiation filling all space.

The Emission of Energy as Electromagnetic Waves or As Moving Subatomic Particles, Especially High-Energy Particles Which Cause Ionization.

 

 

  • Track 12-1Ionizing radiation
  • Track 12-2Particle radiation
  • Track 12-3Gravitational radiation
  • Track 12-4Gravitational wave background (GWB)
  • Track 12-5Cosmic microwave background (CMB)
  • Track 12-6Cosmic neutrino background (CNB)
  • Track 12-7Cosmic infrared background (INB)

Particle physics is a division of physics that studies the nature of the particles that establish matter and radiation. Although the word atom can refer to various types of very small objects, particle physics usually investigates the irreducibly smallest obvious particles and the important interactions necessary to clarify their behaviour.

The Higgs boson is an elementary particle in the Standard Model of particle physics, produced by the quantum excitation of the Higgs field, one of the fields in particle physics theory.

 

  • Track 13-1Observed elementary bosons
  • Track 13-2Gauge bosons
  • Track 13-3 W and Z bosons
  • Track 13-4 W and Z bosons
  • Track 13-5Scalar boson

Asteroids and comets are considered remnants from the huge cloud of gas and dust that condensed to generate the sun, planets, and moons certain 4.5 billion years ago. Today, most asteroids orbit the sun in a tightly packed belt located between Mars and Jupiter. And when detected through a telescope, comets appear fuzzier.

 

  • Track 14-1Hyperbolic comets
  • Track 14-2The C-type asteroids
  • Track 14-3The S-types asteroids
  • Track 14-4The M-types asteroids
  • Track 14-5Massive planet
  • Track 14-6Extrasolar planet
  • Track 14-7Metallic dusts
  • Track 14-8 Mineral dusts
  • Track 14-9Chemical dusts
  • Track 14-10Organic and vegetable dusts

A neutrino is a subatomic subdivision that is very like to an electron, but has no electrical charge and a very minor mass, which might even be zero. Neutrinos are one of the most plentiful particles in the universe.

Nuclear astrophysics is the study of nuclear-level procedures that happen naturally in space. Notably, this comprises understanding the chain of synthesis events, or nucleosynthesis, that occurs in stars, and how this can be noticed from a distance by gauging the radiation these processes produce.

 

 

 

  • Track 15-1Electron Neutrino
  • Track 15-2 Muon Neutrino
  • Track 15-3Tau Neutrino
  • Track 15-4Nuclear physics
  • Track 15-5Nucleosynthesis
  • Track 15-6Abundance of the chemical elements
  • Track 15-7Joint Institute for Nuclear Astrophysics

Astrophysics is that the branch of natural philosophy that deals with the physics of the universe, particularly with “the nature of the heavenly bodies, instead of their positions or motions in space”. Among the objects studied area unit galaxies, stars, planets, additional star planets, the interstellar space and also the cosmic microwave background. 

Gravitational waves are disturbances within the curvature of area time, generated by accelerated plenty that propagate as waves outward from their supply at the speed of sunshine. Attractive force waves transport energy as attractive force radiation, a variety of energy just like no particulate radiation. 

 

  • Track 16-1Quantum gravity, wave-particle aspects, and graviton
  • Track 16-2Gravitational wave astronomy
  • Track 16-3 Gravitational radiation
  • Track 16-4Black hole binaries
  • Track 16-5Spinning neutron stars
  • Track 16-6Observational astrophysics
  • Track 16-7Theoretical astrophysics

Electromagnetic radiation may be a style of energy that's all around America and takes several procedures, like radio waves, microwaves, X-rays and gamma rays. Daylight is additionally a style of EM energy, however visible radiation is barely a little portion of the EM spectrum, that contains a broad vary of magnetism wavelengths.

 

  • Track 17-1Radio Waves
  • Track 17-2Microwaves
  • Track 17-3Infrared radiation
  • Track 17-4Visible Light

Aeronautics is that the science or art attached the study, design, and producing of air flight capable machines, and also the techniques of operative craft and rockets at intervals the atmosphere. British Royal physics Society identifies the aspects of "aeronautical Art, Science and Engineering" and "the profession of physics (which expression includes Astronautics)." whereas the term originally referred only to operative the craft, it's since been enlarged to incorporate technology, business, and different aspects associated with craft.

Aerospace engineering is that the primary field of engineering involved with the event of craft and satellite. Its 2 major and superimposed branches: natural philosophy engineering and astronautically engineering. Aeronautics engineering is analogous, however deals with the semiconductor unit technology aspect of part engineering.

 

  • Track 18-1Aeronautical engineering
  • Track 18-2Astronautical engineering
  • Track 18-3Avionics engineering
  • Track 18-4Aeronautical science
  • Track 18-5Balloon flight
  • Track 18-6Cayley and the foundation of modern aeronautics
  • Track 18-7Aerodynamics

Physics is the subdivision of science that contracts with the structure of substance and how the important ingredients of the universe interrelate. It studies objects reaching from the very minor using quantum mechanics to the whole universe using general relativeness the study 0f matter, energy and their communications - is an international enterprise, which plays a key role in the future development of humankind.

Astronomy is that the scientific change of heavenly matters like stars, planets, comets, and galaxies and phenomena that originate outside the Earth's atmosphere like the cosmic background. It’s distressed with the evolution, physics, chemistry, meteorology, and motion of celestial objects, additionally because the development and enlargement of the universe. Uranology is one among the hoariest sciences. Astronomers of early developments did systematic observations of the night sky, and astronomical artifacts are originated from a lot of previous periods.

 

  • Track 19-1Quantum physics
  • Track 19-2Chemical physics
  • Track 19-3Observational astronomy
  • Track 19-4Theoretical astronomy
  • Track 19-5Amateur astronomy
  • Track 19-6Unsolved problems in astronomy

Cosmology could be a branch of physics involved with the studies of the origin and evolution of the universe, from the massive bang to these days and on into the long run. It’s the scientific study of the origin, evolution, and ultimate fate of the universe

  • Track 20-1Physical cosmology
  • Track 20-2Religious cosmology
  • Track 20-3Metaphysical cosmology
  • Track 20-4Esoteric cosmology

Astrochemistry is that the study of the copiousness and reactions of molecules within the Universe, and their interaction with radiation. The correction is associate degree overlap of natural philosophy and chemistry. The word "astrochemistry" could also be realistic to each the system and also the interstellar space. Astrochemistry is associate degree knowledge base space of data at the intersection between chemistry and natural philosophy. 

Spectroscopy is the study of the interaction between matter and electromagnetic radiation. Historically, spectroscopy originated through the study of visible light dispersed according to its wavelength, by a prism.

 

 

  • Track 21-1Space chemistry
  • Track 21-2Chemical Reactions in astrochemistry
  • Track 21-3Chemical Kinetics in astrochemistry
  • Track 21-4Chemical Bonding in astrochemistry
  • Track 21-5Structure/Functions changes in astrochemistry
  • Track 21-6Inter-molecular Interactions in astrochemistry
  • Track 21-7Atomic Spectroscopy
  • Track 21-8Ultraviolet and Visible Spectroscopy
  • Track 21-9Infrared Spectroscopy
  • Track 21-10Raman Spectroscopy
  • Track 21-11Nuclear Magnetic Resonance