If you've never seen a real, live spacecraft orbiting the earth, well now's your chance! The Russian space station Mir can easily be spotted with the naked eye, and in fact is brighter than most of the stars you can see. You would probably mistake it for an airplane if you didn't know better--except that it has no little blinking lights, and it doesn't make any noise!

Mir is visible because of the sunlight that reflects off it. That means that certain conditions must exist before we on earth can see it:

Because of this, the times you're most likely to see Mir are for a little while after sunset, and a little while before sunrise. At other times, either our sky will be too bright, or Mir will likely be in the earth's shadow.

Mir's orbit on May 26, 1998
And of course, the other condition is that Mir has to be flying over your part of the earth at the time! Fortunately, Mir is in a "high-inclination" orbit, which means it reaches far northern and southern latitudes. This orbit, combined with the earth's rotation, means that Mir passes over most places on the earth fairly regularly (typically several times each day, for any given spot). On average, the lighting conditions at your location will be right for viewing every few days or so. However, during certain auspicious times around summer, when Mir's orbit lines up pretty closely with the earth's "terminator" (the dividing line between the earth's light & dark half), Mir can actually remain in sunlight during its entire orbit. At times like that, it may be visible as much as three or four times in a single night!

Most people are surprised to see how fast Mir moves through the sky. When it's passing directly overhead, if you hold your hand out at arm's length, Mir will cross the width of three fingers in about five seconds. It's traveled about 25 miles in that time!

Viewing Tips
You can often see Mir through binoculars even when it's too dim to see with the naked eye. The following things affect its visibility:

How far away is it?
Mir orbits at an altitude of about 235 miles (sometimes a little more, sometimes a little less, because its orbit is not a perfect circle). But its distance away from you could be a great deal more than that, depending on its angle above the horizon (see the illustration above). This angle is called the "elevation angle" or the "altitude angle," and ranges from 0° (right on the horizon) to 90° (directly overhead). If you know this angle, you can get a good estimate of Mir's "Line-of-sight" distance. See the table.

Is it over my city?
The "Ground-track distance" is the distance along the ground between your position and the spot that's directly underneath Mir. If you know the ground-track distance and the compass direction to Mir, then you can look on a map to see what city it's passing over. The ground-track distance can be estimated from Mir's elevation angle: see the table.

Visibility Predictions

This section will be updated every week or so with charts for predicted sightings of Mir from selected cities (selected because I have friends and family who live there :-). If your city is not on this list, check out these excellent sites:

If your Web browser can run Java programs, then try NASA's J-Pass program. It predicts the visibility of Mir and dozens of other satellites from many cities, and even lets you enter your own latitude and longitude if your city's not listed. It even draws charts (not as pretty as mine, though :-).

How to read the charts
The red arc shows Mir's predicted path through the sky. The time displayed in the corner of the chart shows roughly the time at which Mir will first become visible; at that time, it will show up at one end of the arc (at the end labeled "Mir,") and will begin moving toward the other end. The red dots on the arc show Mir's position at 1-minute intervals.

The scale of these charts varies greatly. Use the grid lines to get an accurate idea of how much of the sky is involved:

Mir always moves more or less west to east: in some charts, that will be left to right; in others, right to left (depending on whether it's in the northern or southern part of the sky). Compass directions are displayed along the horizon.

You may notice that sometimes the "path" seems to start or end while Mir is still high in the sky. This usually means that Mir is entering or leaving the earth's shadow at that point. (This actually looks pretty cool--you can watch Mir "fade in" or "fade out" in a matter of just a couple of seconds).

Predictions for Sunday, July 26 through Sunday, August 2, 1998
These lists show the date and local time of the beginning of the sighting, and the maximum elevation above the horizon that Mir will reach (I haven't included any sightings that don't get above about 30°, because they're very hard to see). Just click on any listed sighting to see its chart. All of these charts were generated using Sienna Software's "Starry Night Deluxe" program.

Click on a city name to generate a 10-day forecast that also includes low-elevation passes.

More Mir Links