Zitat:An all-sky view of stars in our Galaxy – the Milky Way – and neighbouring galaxies, based on the first year of observations from ESA’s Gaia satellite, from July 2014 to September 2015.
This map shows the density of stars observed by Gaia in each portion of the sky. Brighter regions indicate denser concentrations of stars, while darker regions correspond to patches of the sky where fewer stars are observed.
The Milky Way is a spiral galaxy, with most of its stars residing in a disc about 100 000 light-years across and about 1000 light-years thick. This structure is visible in the sky as the Galactic Plane – the brightest portion of this image –which runs horizontally and is especially bright at the centre.
Darker regions across the Galactic Plane correspond to dense clouds of interstellar gas and dust that absorb starlight along the line of sight.
Many globular and open clusters – groupings of stars held together by their mutual gravity – are also sprinkled across the image.
Globular clusters, large assemblies of hundreds of thousands to millions of old stars, are mainly found in the halo of the Milky Way, a roughly spherical structure with a radius of about 100 000 light-years, and so are visible across the image.
Open clusters are smaller assemblies of hundreds to thousands of stars and are found mainly in the Galactic Plane.
The two bright objects in the lower right of the image are the Large and Small Magellanic Clouds, two dwarf galaxies orbiting the Milky Way. Other nearby galaxies are also visible, most notably Andromeda (also known as M31), the largest galactic neighbour to the Milky Way, in the lower left of the image. Below Andromeda is its satellite, the Triangulum galaxy (M33).
A number of artefacts are also visible on the image. These curved features and darker stripes are not of astronomical origin but rather reflect Gaia’s scanning procedure. As this map is based on observations performed during the mission’s first year, the survey is not yet uniform across the sky.
These artefacts will gradually disappear as more data are gathered during the five-year mission.

http://www.esa.int/spaceinimages/Images/..._annotated

Zitat:Hast Du schon mal recherchiert, wo das Ding runter kommt, weil der Anblick eines solchen Brocken's ist schon beeindruckend.

Zitat:Latest Re-Entry Predictions:
Spaceflight101: May 10, 2015 - 12:15 UTC +/-3 Days [Issued: May 1]
Satflare/Joseph Remis: May 10, 2015 - 17:05 UTC +/-52 Hours [Issued May 1]
USSTRATCOM: May 9, 2015 - 17:33 UTC +/-6 Days [Issued: April 29, 17:47]
Roscosmos: Initially: May 7-11, Revised: May 5-7 [Issued: April 29]
ESA: May 9, 2015 +/-2 Days [Issued: April 30]

Zitat:Am 6. März 2015 wird die Raumsonde Dawn von der Schwerkraft des Zwergplaneten Ceres eingefangen. Gegen Ende April wird die Sonde mit der ersten Detailkartierung beginnen. Die neuesten Bilder des Zwergplaneten unterstützen den Eindruck einer Kraterwüste, aber es gibt auch spannende Hinweise auf innere geologische Aktivität.

Zitat:11.11.2014, 19:33 MEZ: Der Lander wird eingeschaltet.
11.11.2014, 20:30 MEZ: GO/NOGO-Entscheidung Nr. 1. Wenn die Bahn von Rosetta nun korrekt ist, läuft alles weiter.
12.11.2014, 01:00 MEZ: GO/NOGO-Entscheidung Nr. 2. Wenn Rosetta so funktioniert, wie sie soll, läuft die Mission weiter.
12.11.2014, 02:35 MEZ: GO/NOGO-Entscheidung Nr. 3. Wenn Philae bereit ist, kann es weiter gehen.
12.11.2014, 08:35 MEZ: Spätestmöglicher Zeitpunkt für die letzte GO/NOGO-Entscheidung die bestimmt, ob die Landung eingeleitet wird oder nicht.
12.11.2014: 10:03 MEZ: Nachdem sich Philae von Rosetta gelöst hat und zum Kometen absteigt, dauert es ein wenig, bis das bestätigende Signal auf der Erde eingetroffen ist. Es sollte gegen 10 Uhr ankommen.
12.11.2014, 11:53 MEZ: Bestätigung der geglückten Kommunikation zwischen Rosetta und Philae. Ohne diese Verbindung kann Philae keine Signale zur Erde schicken.
12.11.2014, 17:02 MEZ: Landung auf dem Kometen!