Skylights featured on Astronomy Picture of the Day |
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Skylights featured eight times on Earth Science Picture of the Day: 1 2 3 4 5 6 7 8 |
| Go to STARS for previous stars of the week. | Last week's Skylights is still available. | Access Skylights' Archive and photo gallery. | Find out what happened in astronomy at Astronomy Updates. |
| The Constellations has a linked list with locations and brightest stars. | Constellation Maps show the locations of the constellations. | The 151 Brightest Stars lists through magnitude 2.90. | For more on stars and constellations, visit Stellar Stories. |
| Watch a total eclipse of the Moon and an annular eclipse of the Sun. | Moon Light presents photos of the Moon. | See the Moon move and pass just below Nu Virginis. | Watch planets move against the background stars. |
| See a classic proof of the curvature of the Earth with a "hull down" series. | Visit Measuring the Sky to learn about the celestial sphere. | Admire sunsets, rainbows, and other sky phenomena in Sunlight. | Go from Day Into Night, with 83 linked illustrations. |
| See the The Aurora and the Midnight Sun. | Take a ride aboard Asteroid 17851 Kaler (1998 JK). | Look for Books about the sky and stars. | ![]() |
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78 Ursae Majoris B goes around 78 UMa A (the brighter and more massive of the two, placed at the cross) with a period of 106 years at an average separation of 31 1/4 Astronomical Units. Observations (the colored points) are missing where the stars were too close together. Tilted through a 50 degree angle to the plane of the sky, the orbit is quite noticeably foreshortened, as can be seen by the off-center displacement of the true ellipse's major axis (the dot-dash line). The arrow at lower right shows the direction of motion. Double star observers measure the position of the fainter star relative to the brighter rather than the actual motions of both stars around the common center of mass that lies between them. North is down, as would be seen in a telescope. The scales around the edges are in seconds of arc. (From an article by M. Scardia et al. in the Monthly Notices of the Royal Astronomical Society, vol. 357, p. 1255, 2005, image courtesy of W. I. Hartkopf.) |