OrbitalHub

NASA dixit:

“A new study using data from NASA’s NuSTAR space telescope suggests that the most luminous and massive stellar system within 10,000 light-years, Eta Carinae, is accelerating particles to high energies — some of which may reach Earth as cosmic rays. Cosmic rays with energies greater than 1 billion electron volts (eV) come to us from beyond our solar system. But because these particles — electrons, protons and atomic nuclei — all carry an electrical charge, they veer off course whenever they encounter magnetic fields. This scrambles their paths and masks their origins. Eta Carinae, located about 7,500 light-years away in the southern constellation of Carina, contains a pair of massive stars whose eccentric orbits bring them unusually close every 5.5 years. The stars contain 90 and 30 times the mass of our Sun.

Both stars drive powerful outflows called stellar winds, which emit low-energy X-rays where they collide. NASA’s Fermi Gamma-ray Space Telescope observes gamma rays — light packing far more energy than X-rays — from a source in the direction of Eta Carinae. But Fermi’s vision isn’t as sharp as X-ray telescopes, so astronomers couldn’t confirm the connection. To bridge this gap, astronomers turned to NASA’s NuSTAR observatory. Launched in 2012, NuSTAR can focus X-rays of much greater energy than any previous telescope.

The team examined NuSTAR observations acquired between March 2014 and June 2016, along with lower-energy X-ray observations from the European Space Agency’s XMM-Newton satellite over the same period. NuSTAR detects a source emitting X-rays above 30,000 eV, some three times higher than can be explained by shock waves in the colliding winds. For comparison, the energy of visible light ranges from about 2 to 3 eV.

The researchers say both the X-ray emission seen by NuSTAR and the gamma-ray emission seen by Fermi is best explained by electrons accelerated in shock waves where the winds collide. The X-rays detected by NuSTAR and the gamma rays detected by Fermi arise from starlight given a huge energy boost by interactions with these electrons. Some of the superfast electrons, as well as other accelerated particles, must escape the system and perhaps some eventually wander to Earth, where they may be detected as cosmic rays. Zoom into Eta Carinae, where the outflows of two massive stars collide and shoot accelerated particles cosmic rays into space.”

Credits Music: “Expectant Aspect” from Killer Tracks

Credits Video: NASA’s Goddard Space Flight Center

Wikipedia dixit:

“The James Webb Space Telescope (JWST) is a space telescope developed in collaboration between NASA, the European Space Agency, and the Canadian Space Agency that will be the scientific successor to the Hubble Space Telescope. The JWST will offer unprecedented resolution and sensitivity, and will enable a broad range of investigations across the fields of astronomy and cosmology. One of its major goals is observing some of the most distant events and objects in the universe, such as the formation of the first galaxies. These types of targets are beyond the reach of current ground and space-based instruments. Other goals include understanding the formation of stars and planets, and direct imaging of exoplanets and novas.

The JWST’s primary mirror is composed of 18 hexagonal mirror segments made of gold-coated beryllium that combine to create a mirror with a diameter of 6.5 meters (21 ft 4 in) – a large increase over the Hubble’s 2.4-meter (7.9 ft) mirror. The telescope will be deployed in space near the Earth–Sun L2 Lagrangian point, and a large sunshield made of five sheets of silicon- and aluminum-coated Kapton will keep JWST’s mirror and four science instruments below 50 K (−220 °C; −370 °F). Unlike the Hubble—which observes in the near ultraviolet, visible, and near infrared spectra—the JWST will observe in the long-wavelength (orange to red) visible light through the mid-infrared (0.6 to 27 μm) range. This will allow the JWST to observe high redshift objects that are too old and too distant for the Hubble and other earlier instruments to observe.

In development since 1996, the telescope is named after James E. Webb, the American government official who was the administrator of NASA from 1961 to 1968 and played an integral role in the Apollo program. The project has had numerous delays and cost overruns, and underwent a major redesign during 2005. In December 2016, NASA announced that construction of the JWST was complete and that its extensive testing phase would begin. In March 2018, NASA delayed the JWST’s launch an additional year after the telescope’s sunshield ripped during a practice deployment and the sunshield’s cables did not sufficiently tighten. It was further delayed on June 27, 2018 based on recommendations by an Independent Review Board. The JWST is scheduled to launch on March 30, 2021.”

Credits Video: NASA/Northrop Grumman

Wikipedia dixit:

“The James Webb Space Telescope (JWST) is a space telescope developed in collaboration between NASA, the European Space Agency, and the Canadian Space Agency that will be the scientific successor to the Hubble Space Telescope. The JWST will offer unprecedented resolution and sensitivity, and will enable a broad range of investigations across the fields of astronomy and cosmology. One of its major goals is observing some of the most distant events and objects in the universe, such as the formation of the first galaxies. These types of targets are beyond the reach of current ground and space-based instruments. Other goals include understanding the formation of stars and planets, and direct imaging of exoplanets and novas.

The JWST’s primary mirror is composed of 18 hexagonal mirror segments made of gold-coated beryllium that combine to create a mirror with a diameter of 6.5 meters (21 ft 4 in) – a large increase over the Hubble’s 2.4-meter (7.9 ft) mirror. The telescope will be deployed in space near the Earth–Sun L2 Lagrangian point, and a large sunshield made of five sheets of silicon- and aluminum-coated Kapton will keep JWST’s mirror and four science instruments below 50 K (−220 °C; −370 °F). Unlike the Hubble—which observes in the near ultraviolet, visible, and near infrared spectra—the JWST will observe in the long-wavelength (orange to red) visible light through the mid-infrared (0.6 to 27 μm) range. This will allow the JWST to observe high redshift objects that are too old and too distant for the Hubble and other earlier instruments to observe.

In development since 1996, the telescope is named after James E. Webb, the American government official who was the administrator of NASA from 1961 to 1968 and played an integral role in the Apollo program. The project has had numerous delays and cost overruns, and underwent a major redesign during 2005. In December 2016, NASA announced that construction of the JWST was complete and that its extensive testing phase would begin. In March 2018, NASA delayed the JWST’s launch an additional year after the telescope’s sunshield ripped during a practice deployment and the sunshield’s cables did not sufficiently tighten. It was further delayed on June 27, 2018 based on recommendations by an Independent Review Board. The JWST is scheduled to launch on March 30, 2021.”

Credits Music: Expanding Time and Space by Daniel jay Nielsen

Credits Video: NASA’s Goddard Space Flight Center/Sophia Roberts

ESA dixit:

“This is a 360° animated view of the entire sky. After a few seconds, the stars start moving in the sky according to parallax, an apparent shift caused by Earth’s yearly motion around the Sun. Then, constellation outlines appear as visual aids. Finally, stars start moving according to their true motion through space, which is visible on the sky as proper motion. Parallaxes have been exaggerated by 100 000 and proper motions have been speeded up by one trillion (10^12) to make them visible in this animation. This animation is based on data from the second data release of ESA’s Gaia satellite, which has measured the positions, parallaxes and motions of more than one billion stars across the sky to unprecedented accuracy. “

Credits Video: ESA/Gaia/DPAC, CC BY SA 3.0 IGO/Gaia Data Processing and Analysis Consortium (DPAC); Gaia Sky; S. Jordan/T. Sagristà, Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Germany

ESA dixit:

“The second data release of ESA’s Gaia mission has produced an extraordinary catalogue of over one and a half billion stars in our galaxy. Based on observations between July 2014 to May 2016, it includes the most accurate information yet on the positions, brightness, distance, motion, colour and temperature of stars in the Milky Way as well as information on asteroids and quasars.”

Credits Video:ESA

ESA dixit:

“This is an animated view of the 14 099 asteroids in our Solar System, as viewed by ESA’s Gaia satellite using information from the mission’s second data release. The orbits of the 200 brightest asteroids are also shown, as determined using Gaia data. In future data releases, Gaia will also provide asteroid spectra and enable a complete characterisation of the asteroid belt. The combination of dynamical and physical information that is being collected by Gaia provides an unprecedented opportunity to improve our understanding of the origin and the evolution of the Solar System. “

Credits Video: ESA / Gaia / DPAC / Gaia Data Processing and Analysis Consortium (DPAC); Orbits: Gaia Coordinating Unit 4; P. Tanga, Observatoire de la Côte d’Azur, France; F. Spoto, IMCCE, Observatoire de Paris, France; Animation: Gaia Sky; S. Jordan / T. Sagristà, Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Germany