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Exoplanets around the pulsar PSR B1257+12: PSR B1257+12, also called Lich since December 2015, is a pulsar located at a distance of 2300 light years from the Sun, in the constellation of the Virgin. In 1992 two planets orbiting the star were discovered. A third planet was discovered later around PSR B1257+12. PSR B1257+12, also named Lich, is a pulsar located 2300 light years from the Sun in the constellation of Virgo. The pulsar has a planetary system with three known extrasolar planets, named “” Draugr”” (PSR B1257+12 A), “” Poltergeist”” (PSR B1257+12 B) and “” Phobetor””” (PSR B1257+12 C), respectively. They were both the first extrasolar planets and the first pulsar planets to be discovered; A and B in 1992 and C in 1994

Exoplanets around the pulsar PSR B1257+12: PSR B1257+12, also called Lich since December 2015, is a pulsar located at a distance of 2300 light years from the Sun, in the constellation of the Virgin. In 1992 two planets orbiting the star were discovered. A third planet was discovered later around PSR B1257+12. PSR B1257+12, also named Lich, is a pulsar located 2300 light years from the Sun in the constellation of Virgo. The pulsar has a planetary system with three known extrasolar planets, named “” Draugr”” (PSR B1257+12 A), “” Poltergeist”” (PSR B1257+12 B) and “” Phobetor””” (PSR B1257+12 C), respectively. They were both the first extrasolar planets and the first pulsar planets to be discovered; A and B in 1992 and C in 1994

Miller, Ron (b.1947)

PIX4608544

Aristide Briand during a speech before the League of Nations, 1926 (b/w photo)

Aristide Briand during a speech before the League of Nations, 1926 (b/w photo)

SZT2991710

Aristide Briand (b/w photo)

Aristide Briand (b/w photo)

SZT2991747

Exoplanete PSR B1620-26 b - Mathusalem - Exoplanet PSR B1620-26 b - Methuselah: PSR B1620-26 b, unofficially nicknamed Mathusalem is a circumbinary exoplanet of about 2.5 Jovian masses. It would be the oldest known planet, perhaps 13 billion years old. Discovered in 1993 around the binary system formed by PSR B1620-26 and WD B1620-26, respectively a pulsar and a white dwarf orbiting around each other. This system is approximately 12,400 light-years away from Earth in the M4 globular cluster of the constellation Scorpio. PSR B1620-26 b is an extrasolar planet located approximately 12,400 light-years away from Earth in the constellation of Scorpius. It bears the unofficial nickname “” Methuselah”” due to its extreme age. The planet is in a circumbinary orbit around a pulsar (PSR B1620-26) and a white dwarf (WD B1620-26)) and is the first circumbinary planet ever confirmed. It is also the first planet found in a globular cluster. The planet is one of the oldest known extrasolar planets, b

Exoplanete PSR B1620-26 b - Mathusalem - Exoplanet PSR B1620-26 b - Methuselah: PSR B1620-26 b, unofficially nicknamed Mathusalem is a circumbinary exoplanet of about 2.5 Jovian masses. It would be the oldest known planet, perhaps 13 billion years old. Discovered in 1993 around the binary system formed by PSR B1620-26 and WD B1620-26, respectively a pulsar and a white dwarf orbiting around each other. This system is approximately 12,400 light-years away from Earth in the M4 globular cluster of the constellation Scorpio. PSR B1620-26 b is an extrasolar planet located approximately 12,400 light-years away from Earth in the constellation of Scorpius. It bears the unofficial nickname “” Methuselah”” due to its extreme age. The planet is in a circumbinary orbit around a pulsar (PSR B1620-26) and a white dwarf (WD B1620-26)) and is the first circumbinary planet ever confirmed. It is also the first planet found in a globular cluster. The planet is one of the oldest known extrasolar planets, b

Miller, Ron (b.1947)

PIX4608526

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

PIX4572892

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of

PIX4572795

White dwarf and planet in the globular cluster M4 - Oldest known planet in globular cluster M4 - The globular cluster M4 is located about 7000 years from Earth and seems to be 13 billion years old. The Hubble a space telescope identifies a Jupiter-sized planet orbiting a white dwarf star (arrow on the image). It would be the oldest planet known to date. Hubble Space Telescope image of stars in globular cluster M4. Marked is a white - dwarf star, which is orbited by the pulsar called PSR B1620 - 26; this system had been discovered by radio astronomers in 1988. Only the white dwarf is visible in this image. The system has a third companion, it has a mass 2.5 times larger than planet Jupiter, and is thus recognized as a planet

White dwarf and planet in the globular cluster M4 - Oldest known planet in globular cluster M4 - The globular cluster M4 is located about 7000 years from Earth and seems to be 13 billion years old. The Hubble a space telescope identifies a Jupiter-sized planet orbiting a white dwarf star (arrow on the image). It would be the oldest planet known to date. Hubble Space Telescope image of stars in globular cluster M4. Marked is a white - dwarf star, which is orbited by the pulsar called PSR B1620 - 26; this system had been discovered by radio astronomers in 1988. Only the white dwarf is visible in this image. The system has a third companion, it has a mass 2.5 times larger than planet Jupiter, and is thus recognized as a planet

PIX4564537

The Gamma ray sky - The Gamma ray sky - Map of the whole sky seen in gamma rays by the Fermi Gamma-Ray Space Telescope (FGST) satellite from August 4 to October 30, 2008. The strongest sources of gamma radiation are legendeed here. All-sky image seen in gamma ray showing the glowing gas of the Milky Way, blinking pulsars, and galaxies billions of light-years away. The all-sky image released today shows us how the cosmos would look if our eyes could detect radiation 150 million times more energetic than visible light. The view merges Large Area Telescope (LAT) on Fermi Gamma-ray Space Telescope (FGST) observations spanning 87 days, from August 4 to October 30, 2008. The top five sources within our galaxy are: The sun. Now near the minimum of its activity cycle, the sun would not be a particularly notable source except for one thing: It's the only one that moves across the sky. The sun's annual motion against the background sky is a reflection of Earth's orbit around the sun. LSI+61 303.

The Gamma ray sky - The Gamma ray sky - Map of the whole sky seen in gamma rays by the Fermi Gamma-Ray Space Telescope (FGST) satellite from August 4 to October 30, 2008. The strongest sources of gamma radiation are legendeed here. All-sky image seen in gamma ray showing the glowing gas of the Milky Way, blinking pulsars, and galaxies billions of light-years away. The all-sky image released today shows us how the cosmos would look if our eyes could detect radiation 150 million times more energetic than visible light. The view merges Large Area Telescope (LAT) on Fermi Gamma-ray Space Telescope (FGST) observations spanning 87 days, from August 4 to October 30, 2008. The top five sources within our galaxy are: The sun. Now near the minimum of its activity cycle, the sun would not be a particularly notable source except for one thing: It's the only one that moves across the sky. The sun's annual motion against the background sky is a reflection of Earth's orbit around the sun. LSI+61 303.

PIX4638007

Poster of the referendum on the Dissolution of the Prussian Landtag, 1931

Poster of the referendum on the Dissolution of the Prussian Landtag, 1931

SZT5177601

Joseph Goebbels and Wilhelm Weiss at the Reich Press Day in Berlin, 1934 (b/w photo)

Joseph Goebbels and Wilhelm Weiss at the Reich Press Day in Berlin, 1934 (b/w photo)

Scherl

SZT6363376

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