Trying to
observe near the sun is difficult, but a planet is not exactly an easy thing to hide.
Not exact matches
In fact, from each ocean view room balcony hotel guests can
observe the
near constant clutch of surfers hanging ten — a quintessentially Californian vista, especially as they are silhouetted at dusk against the orange, red and otherwise polychromatic backdrop of the setting
sun.
This was first confirmed during a solar eclipse in 1919 by a team led by the British astronomer Arthur Eddington; the scientists
observed that stars
near the limb of the
Sun were shifted in position by the
Sun's gravity.
On our star, the
Sun, the sunspots are seen in a belt around the equator, but now scientists have
observed a large, distant star where sunspots are located
near the poles.
We now have to
observe how the coma evolves as it
nears the
sun, to determine whether the changes in the coma are a result of temperature differences alone or whether the nucleus itself is inhomogeneous.»
The image above (view the full - res version), which is called the absorption spectrum of the
Sun, was
observed by the Fourier Transform Spectrometer at the National Solar Observatory on Kitt Peak,
near Tucson, Arizona.
That effect was first demonstrated during a total solar eclipse in 1919, when the positions of stars
near the
Sun were
observed to be slightly shifted from their usual positions — an effect due to the pull of the
Sun's gravity as the stars» light passed close to the
Sun.
Besides these remote organizations, investigators have
observed what appear to be groups of high - velocity stars
near the
Sun.
The best -
observed dust clouds
near the
Sun have masses of several hundred solar masses and sizes ranging from a maximum of about 200 light - years to a fraction of a light - year.
This was first tested in 1919 by Sir Arthur Eddington, who organized an expedition to
observe star positions during an eclipse of the
Sun from islands
near the coast of Africa.
«We're accustomed to seeing how our
Sun appears in visible light, but that can only tell us so much about the dynamic surface and energetic atmosphere of our
nearest star,» said Tim Bastian, an astronomer with the National Radio Astronomy Observatory in Charlottesville, Va. «To fully understand the
Sun, we need to study it across the entire electromagnetic spectrum, including the millimeter and submillimeter portion that ALMA can
observe.»
On the other hand,
observing that things warm up during the day, and cool down at night, might cause one to come to the conclusion that objects exposed to the
Sun tend to warm, and that objects exposed to the
near vacuum of outer space tend to lose energy, and cool.
Mancke designed the
Sun Hive after having
observed a wild bee nest in the woods
near his home, which took an egg - shaped form and was covered in waxy skin and propolis.