StarDate

The crescent Moon charges through a rapidly disappearing group of bright stars and planets early this evening. Most of the group will be gone from view by the end of the month.

As twilight begins to fade, the planet Mercury is close below the Moon. Brighter Jupiter is the same distance to the left or upper left of the Moon. Pollux and Castor, the twins of Gemini, are to the upper right of the Moon. And the brightest member of the group is farther to the upper left of the Moon: Venus, the brilliant “evening star.”

Except for Venus, all the members of the group are dropping toward the Sun as seen from Earth. For Pollux and Castor, it’s because all true stars rise and set four minutes earlier each day. So every star disappears in the evening twilight at the same time every year.

For Jupiter and Mercury, the descent is due in part to the same thing – the daily shift of the starry background. But it’s also influenced by the relative motions of Earth and the planets themselves. Mercury is beginning a rapid dive toward the Sun, and will cross between Earth and Sun in a few weeks. Jupiter, on the other hand, is headed toward a passage behind the Sun as seen from Earth.

But Venus is actually moving farther from the Sun. It won’t reach its peak separation for two months, so it’ll remain in good view in the western evening sky into October.

We’ll have more about the Moon and Venus tomorrow.

Script by Damond Benningfield

Like a cosmic butterfly, a cluster of young stars is just emerging from its cocoon – a cloud of gas and dust. The cocoon `spans about 45 light-years. But some of the beautiful butterfly is already in view. Parts of the gas cloud are lit up by the brightest of the infant stars taking shape there. That creates a glowing patch of red and blue.

The whole complex is known as the Cocoon Nebula. It’s about 4,000 light-years away, in Cygnus. Hundreds of stars are being born inside it.

The most impressive of those stars is about 14 times as massive as the Sun, and tens of thousands of times brighter. It’s especially bright in the ultraviolet – wavelengths that are invisible to the human eye. The U-V zaps atoms of hydrogen in the nebula, splitting them apart. When the atoms re-combine, they emit red light – the main color of the nebula.

The hot star also illuminates dust grains in the nebula. It doesn’t set them aglow; instead, the light simply reflects off the grains. That colors the blue parts of the nebula.

Less-massive stars – stars like the Sun or even smaller – are still coming together. They won’t shine as fully formed stars for millions of years.

The Cocoon Nebula is low in the northeast at nightfall. It’s to the lower left of the bright star Deneb, which marks the tail of the swan. The nebula is too faint to see with the eye alone.

Script by Damond Benningfield

The Sun’s closest planet is making a pretty good appearance in the early evening. As seen from Earth, it’s just about as far from the Sun as it ever gets. It looks like a bright star low in the west-northwest beginning shortly after sunset.

Mercury is getting ready to cross between Earth and the Sun – a point known as inferior conjunction. In the meantime, it’ll drop closer and closer to the Sun as viewed from Earth. It’ll vanish in the twilight in a couple of weeks.

Mercury’s orbit is carrying the planet closer to Earth. Tonight, it’s about 78 million miles away. At conjunction, it’ll close to just 53 million miles.

On average, Mercury returns to conjunction every 116 days. But the gap varies by more than 10 days in either direction. That’s because Mercury’s orbit is more lopsided than that of any other planet. When Mercury is closer to the Sun it moves faster; when it’s farther it moves more slowly. So the gap between conjunctions varies depending on where Mercury is in its orbit when it passes Earth.

For the next few nights, look for Mercury as evening twilight fades. Although the planet is bright, it’s so low that you need a clear horizon to spot it. It lines up to the lower right of the much brighter planets Venus and Jupiter. And the crescent Moon will join the lineup on Tuesday, helping point the way to the little planet.

Script by Damond Benningfield

A relic from the early universe is racing through Libra. It’s moving across the constellation at 800,000 miles per hour. That’s far faster than most of the stars around us. So it’ll move out of Libra in the blink of a cosmic eye.

The star is HD 140283. But it also has a nickname – the Methuselah Star. That’s because it’s probably about 13 billion to 14 billion years old. Since the universe itself is only 13.8 billion years old, that makes the star one of the oldest anywhere.

Astronomers have pieced together several bits of evidence to arrive at that age. The key bit is the star’s composition. It has very low levels of elements that are heavier than hydrogen and helium, the simplest elements. Heavier elements were created in the hearts of stars, then spewed into space when the stars died. Some of these elements then were incorporated into later generations of stars.

HD 140283 has less than half a percent as much iron as the Sun, with slightly higher levels of oxygen and a few other elements. Those abundances tell astronomers the star must have been born when the universe was brand new.

As night falls, the star is to the lower left of Zubeneschamali, Libra’s leading light. It’s too faint to see with the eye alone, but it is visible through binoculars.

Script by Damond Benningfield

Every star in the night sky is moving – orbiting the center of the galaxy. Some are moving toward us, while others are moving away. We can’t see that motion because the stars are so remote. But we can measure it with special instruments – one of the most important techniques in astronomy.

The instruments break the light of a star or other object into its individual wavelengths or colors. Each chemical element imprints its own “barcode” in that array of wavelengths. A star’s motion toward or away from us causes the barcodes to shift position.

If it’s moving away from us, the shift is toward longer, redder wavelengths: a redshift. And if it’s moving toward us, the shift is toward shorter, bluer wavelengths: a blueshift. The size of the shift reveals the speed.

The technique also can reveal how fast a star is spinning; the side that’s rotating toward us is blueshifted, while the opposite side is redshifted. And it can reveal orbiting companions; their gravity pushes and pulls the star, slightly changing its motion.

Two bright stars with well-measured shifts are in view as the sky darkens this evening. Regulus is in the west, well to the upper left of the brilliant planets Venus and Jupiter. Its light is redshifted; it’s moving away from us at about 9300 miles per hour. Antares, quite low in the southeast, is sliding toward us at about 8600 miles per hour – giving its light a definite blueshift.

Script by Damond Benningfield