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Bright star Deneb transits at nightfall

In mid-October each year, the northernmost star of the Summer Triangle, Deneb, transits or climbs to its highest point in the sky at or near 7 p.m. local time (8 p.m. local daylight saving time). What does that mean for skywatchers? Only that this noteworthy star – this beloved member of the Summer Triangle – is shifting ever-westward in our sky as Earth travels around the sun. Its transit at nightfall is a hallmark of the year, marking a shift toward winter – or summer – on your half of the globe.

When the sun or a star transits, it resides at one of three places: at zenith (straight overhead), north of zenith or south of zenith.

At 45 degrees north latitude (St. Paul, Minnesota, or Turin, Italy), Deneb shines straight overhead when it transits.

At 40 degrees north latitude (Denver, Colorado, or Philadelphia, Pennsylvania), Deneb soars to its highest point (about 5 degrees north of zenith) roughly one and one-half hours after sunset, or as evening dusk gives way to nightfall.

The meridian is the imaginary semicircle that arcs across the sky from due north to due south. The sun or any star climbs to its highest point for the day when it crosses your meridian.

At temperate latitudes in the Southern Hemisphere, where it’s now springtime, Deneb transits at or near the same hour by the clock (near 7 p.m. local time). Yet, the sun sets later by the clock at more southerly latitudes, so in the Southern Hemisphere, Deneb at this time of year actually transits at evening dusk, instead of nightfall.

Click here to find out when the sun and Deneb transit in your sky.

At more northerly or southerly latitudes, Deneb either transits to the north or to the south of the zenith point. Appreciably south of 45 degrees north latitude, Deneb lies to the north of the zenith point when it transits; conversely, when Deneb transits at latitudes appreciably north of 45 degrees north latitude, Deneb is viewed in the southern sky.

Two brilliant stars – Vega and Altair – team up with Deneb to complete the humongous Summer Triangle. The luminous Summer Triangle asterism, or star formation, can often be seen in a twilight sky or even from a light-polluted city.

The Great rift of the Milky Way passes through the constellation Cassiopeia and the Summer Triangle. Click here for a larger photo

From mid-northern latitudes, the far-northern stars Deneb and Vega are seen at the “top” of the Summer Triangle whereas the southernmost star Altair is seen at the “bottom.” From the Southern Hemisphere, it’s the other way around: Altair reigns at top and Deneb at bottom. It’s a matter of perspective.

Vega, the Summer Triangle’s westernmost star, is seen to the right of Deneb from mid-northern latitudes. From the Southern Hemisphere, on the other hand, Vega lies to the left of Deneb.

Around the world, the stars of the Summer Triangle transit some four minutes earlier with each following day (or two hours earlier with each following month). So, from northerly latitudes, the Summer Triangle is destined to shift over into the western sky at nightfall as autumn ebbs toward winter … or, for those in the Southern Hemisphere, as spring blooms into summer.

Bottom line: As darkness falls in mid-October, the star Deneb shines at the apex of the sky at mid-northern latitudes.

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Bruce McClure

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