Not exact matches
The
team used NASA's Spitzer Space Telescope along with
observations from telescopes on
Earth, including ESO's Very Large Telescope in Chile and others in Morocco, Hawaii, Spain, and South Africa.
By combining
observations from the ground and in space, the
team observed a plume of low - energy plasma particles that essentially hitches a ride along magnetic field lines — streaming from
Earth's lower atmosphere up to the point, tens of thousands of kilometers above the surface, where the planet's magnetic field connects with that of the sun.
Professor Tingay said the research
team was able to look back through all of the MWA's
observations from November, December and early January, when «Oumuamua was between 95 million and 590 million kilometres from
Earth.
In 1999, he led the
team that made the first
observation of a transiting exoplanet — one that passes directly between its parent star and
Earth.
Some researchers have proposed that these lava floods caused global extinctions on
Earth and that they affect climate change, says planetary geologist Alfred McEwen of the University of Arizona, head of the Io
observation team.
The key
observation from the new research is that the small dip in the HAT - P - 7 b light curve when the planet passes behind its star «is roughly equivalent to the signal of an
Earth - size planet when it passes in front of its parent star,» says Paul Kalas, an astronomer at the University of California, Berkeley, who is not part of the Kepler
team.
He says that one of the more fascinating
observations that RBSPICE has provided his
team involves the injections of ions and electrons from the
Earth's geomagnetic tail into the ring current, which is the large electrical current that surrounds the
Earth.
While there are many debates in regards to how the
Earth's internal evolution is driven, the model created by the
team seemed to find an answer that better fits available
observations and underlying physics.
Using JAMSTEC's supercomputer, the
Earth Simulator, the research
team recreated cold wave forecasts for two cases: 1) when there is more frequent
observation and more data available than usual (as in 2015) and 2) a «normal» year with less data collection from land - based stations and no additional research resources available.
This discovery, and other
observations made by the Penn State
team, provide insight into the complexity of weather and atmospheric composition on exoplanets, and may someday be useful for gauging the habitability of
Earth - size planets.
The
team's
observations — published online today in Astronomy & Astrophysics — pin down 51 Pegasi b's mass (half that of Jupiter's) and the inclination of its orbit (9 ° with respect to
Earth) more accurately than ever before.
Volker Liebig, the director of ESA's
Earth observation programs, notified the FLEX
team of the decision on 18 September, along with
team members from CarbonSat, the other mission up for consideration in the
Earth Explorer 8 competition.
The
team made
observations at many different wavelengths, optimised for different features and cloud layers in Jupiter's atmosphere, to create the first global spectral maps of Jupiter taken from
Earth.
«These environmental and animal
observations are noisy data, so whatever we find, we have to take with a grain of salt,» said Erdem Karaköylü, a Goddard
Earth science data analyst and oceanographer who joined the
team during its expansion.
The intergovernmental Group on
Earth Observations asked Roger Sayre, an ecologist at the US Geological Survey in Reston, Virginia, to lead a
team to categorize terrestrial ecosystems.
The
team measured glacier area change from 1986 to 2014 using satellite images from Landsat, the U.S. Geological Survey's and NASA's
Earth observation programme.
By monitoring a small, nearby star for 11 years with one of the 10 - meter Keck telescopes in Hawaii and combining the data with 4.3 years of similar
observations published by another
team, Vogt and his co-authors found two orbiting planets, with respective masses of at least 3.1 times and seven times the mass of
Earth.
«There's so much that we can learn from close - up spacecraft
observations that we'll never learn from
Earth, as the Pluto flyby demonstrated so spectacularly,» said New Horizons science
team member John Spencer, of the Southwest Research Institute (SwRI) in Boulder, Colo. «The detailed images and other data that New Horizons could obtain from a KBO flyby will revolutionize our understanding of the Kuiper Belt and KBOs.»
The
observations by Dr. Anglada - Escudé's
team have shown that both of the newly discovered planets are «Super-Earths,» which are worlds whose masses can be up to 10 times that of the
Earth.
«This campaign is a
team effort that involves more than a dozen observatories, universities and labs around the globe so we can collectively learn the strengths and limitations of our near -
Earth object
observation capabilities,» he said.
Planets «b, c, and d» - On December 14, 2009, a
team of astronomers (Steven S. Vogt; Robert A. Wittenmyer, R. Paul Butler, Simon O'Toole, Gregory W. Henry, Eugenio J. Rivera, Stefano Meschiari, Gregory Laughlin, C. G. Tinney, Hugh R. A. Jones, Jeremy Bailey, Brad D. Carter, and Konstantin Batygin) announced the discovery of one innermost orbiting super-Earth and two outer - orbiting, Neptune - class planets (with at least 5.1, 18.2, and 24.0 Earth - masses, respectively) in moderately circular, inner orbits around 61 Virginis with periods of 4.2, 38.0, and 124.0 days, based on radial - velocity observations over 4.6 years with the Keck Observatory's High Resolution Echelle Spectrometer (HIRES) and the Anglo - Australian Telescope (U.C. Santa Cruz news release; AAO press release; Keck press release; the Lick - Carnegie Exoplanet Survey Team's «Systemic Console;» and Vogt et al, 20
team of astronomers (Steven S. Vogt; Robert A. Wittenmyer, R. Paul Butler, Simon O'Toole, Gregory W. Henry, Eugenio J. Rivera, Stefano Meschiari, Gregory Laughlin, C. G. Tinney, Hugh R. A. Jones, Jeremy Bailey, Brad D. Carter, and Konstantin Batygin) announced the discovery of one innermost orbiting super-
Earth and two outer - orbiting, Neptune - class planets (with at least 5.1, 18.2, and 24.0
Earth - masses, respectively) in moderately circular, inner orbits around 61 Virginis with periods of 4.2, 38.0, and 124.0 days, based on radial - velocity
observations over 4.6 years with the Keck Observatory's High Resolution Echelle Spectrometer (HIRES) and the Anglo - Australian Telescope (U.C. Santa Cruz news release; AAO press release; Keck press release; the Lick - Carnegie Exoplanet Survey
Team's «Systemic Console;» and Vogt et al, 20
Team's «Systemic Console;» and Vogt et al, 2009).
On May 3, 2007,
team of astronomers (including Jean - Luc Margot; Stan Peale; Igor V. Holin; Raymond F. Jurgens; and Martin A. Slade) announced new evidence that Mercury has a partially molten core using new
observations of fluctuations in Mercury's spin obtained with radar signals bounced off the planet from
Earth (with the 305 - meter Arecibo, the 34 - meter Goldstone, and the 100 - meter Robert C. Byrd Green Bank radio telescopes).
«Interest in
earth observation — and in particular, the value to what we do in development internationally — has never been higher,» said Jenny Frankel - Reed, adaptation
team lead at the U.S. Agency for International Development (USAID).
As others have noted, the IPCC
Team has gone absolutely feral about Salby's research and the most recent paper by Dr Roy Spencer, at the University of Alabama (On the Misdiagnosis of Surface Temperature Feedbacks from Variations in
Earth's Radiant Energy Balance), for one simple reason: both are based on empirical, undoctored satellite
observations, which, depending on the measure required, now extend into the past by up to 32 years, i.e. long enough to begin evaluating real climate trends; whereas much of the
Team's science in AR4 (2007) is based on primitive climate models generated from primitive and potentially unreliable land measurements and proxies, which have been «filtered» to achieve certain artificial realities (There are other more scathing descriptions of this process I won't use).
The
team used radar
observations captured by the European
Earth Remote Sensing (ERS - 1 and -2) satellites to measure just how far the grounding line - the point where the glacier meets the land - had retreated.
WMO workshop participants included high - level representatives of operational and research and development space agencies, the Committee on
Earth Observations Satellites (CEOS), Global Climate Observing System (GCOS), the WMO Space Programme, the WMO Open Programme Area Group / Integrated Observing System (OPAG / IOS), and the Expert
Team on Evolution of the Global Observing System (ET - EGOS).
The
team used newly available NASA satellite
observations of rainfall and vegetation, and a computer model that predicts atmospheric wind flow patterns, to explore the impact of the
Earth's tropical forests.