Hubble Space Telescope’s Galactic Views

Galaxies are fascinating places to explore. They have been around since nearly the beginning of the universe, are home to stars, planets, and other objects. When astronomers look at galaxies, with observatories such as Hubble Space Telescope, they might see star formation regions. They can also observe areas of star death. Many galaxies have black holes, particularly at their cores. And, of course, many stars in galaxies have planets or disks of material in which planets can form. In short, they present fascinating collections of telescope targets to study.

One famous galaxy has even changed our perception of the universe. Another one showed us how much a telescope could be improved. The first happened when astronomer Edwin P. Hubble began studying the Andromeda Galaxy in the 1920s. In 1924, as he observed it, he saw a variable star in one of its spiral arms and took images. Then, he calculated the distance to the galaxy using the period of the star’s brightening and dimming. It was a simple thing to do, but the results reverberated through the astronomy community like a shock wave. And, it forced astronomers to expand their understanding of the size of the universe.

Eventually, astronomy came to grips with the idea of an expanding universe. Astronomers found that galaxies were, indeed, stellar cities of their own. Up until Hubble’s work, they strongly suggested that these fluffy-looking spiral “nebulae” were probably part of our own Milky Way. Hubble’s work changed that forever. In addition, it altered our understanding of the age and extent of the universe.

So, of course, the telescope named after Edwin P. Hubble, the Hubble Space Telescope, has done some of its finest work when looking at galaxies. Whether it’s one galaxy, such as Andromeda, or millions of them (as in the various Deep Field studies it has done), HST regularly cranks out highly detailed views of them.

Hubble Space Telescope’s Grand View of a Grand Design Galaxy

Galaxy M100 has also taught us some lessons. Yesterday, I showed a pic of M100 as the telescope saw it with spherical aberration. Next to it was another one after one of the cameras was outfitted with corrective optics to sharpen the view. Each image of M100 that we’ve seen shows how the venerable and still-flying Hubble Space Telescope has improved.

Hubble turned to look at M100 again after it had an even better camera installed, the Wide Field Camera 3. It was put into the telescope during the last servicing mission in 2009, and almost immediately astronomers turned to M100 to get a better view.

The galaxy M100 as seen by Hubble Space Telescope and the Wide-field Camera 3.
A view of the galaxy M100, taken with the WFC3 camera on board Hubble Space Telescope. Courtesy NASA/ESA/STScI.

Astronomers have long referred to the shape of M100 as a “grand design” galaxy. That’s because it has very obvious spiral arms (two of them!). In the outer regions of the two arms, we can see massive clouds of blue stars. Their presence also makes M100 a starburst galaxy. The region around the core is also blazing with newborn stars. The brownish dust lanes mark regions where stars could form in the future. The core of the galaxy is packed with older stars.

Hubble’s view of M100 resolves individual stars throughout most of this galaxy. Over the years, it has identified Cepheid variables within its arms. Cepheids are stars that vary in a predictable period of time. They have been used to establish cosmic distances since Henrietta Swan Leavitt discovered the period-luminosity relation (in 1908). She came up with that relation by charting their brightening and dimming cycles.

Edwin Hubble used her work to deduce the distance of the Andromeda Galaxy using the Cepheid variable he observed. As I mentioned above, his work showed astronomers that the universe is much larger than they thought at the time. It also gave them a way to more accurately measure distances between galaxies. Other fundamental discoveries about distance and the expansion rate of the universe have flowed from Hubble’s work.

Hubble Views Hubble’s Cepheid: Var!

In May 2011, Hubble Space Telescope turned its gaze toward the galaxy that had so fascinated its namesake. The Andromeda Galaxy is another grand design spiral, and the closest one to our own Milky Way. It lies some 2.5 million light-years away, and it’s moving toward us on a collision course. The 2011 view of Andromeda showed the Cepheid variable star that Hubble measured. It also revealed incredibly sharp images of individual stars. HST’s image gives remarkable insight into Andromeda, which is the only spiral galaxy we can see with the naked eye.

A closeup of the region of the Andromeda Galaxy that contains Hubble's variable star observed in 1931.  Taken by Hubble Space Telescope.
The Hubble Space Telescope imaged the star field around the Cepheid variable V1 in M31. Notice the individual stars, as seen from distance of 2.5 million light-years, along with dust lanes. The blue cluster towards the upper right of the image contains massive young stars that are emitting intense ultraviolet light. The Cepheid variable, V1, the first Cepheid ever found outside of our own galaxy, is a moderate looking star in the lower left of the image. Courtesy NASA/ESA/STScI.

I especially like the comparison view below. It shows a remarkable ground-based view of Andromeda Galaxy, coupled with an inset made by HST (upper right). Edwin P. Hubble’s marked-up plate (lower right) shows the 1924 observation that led to his remarkable discovery. It really shows us how far astronomy has come since Hubble’s day. And, it’s all thanks to his namesake on orbit around Earth.

A ground-based view of the Andromeda Galaxy (left), along with HST’s view of the region around Hubble’s Variable star (marked V1), and the original plate with Hubble’s notation of the variable. Courtesy NASA/ESA/STScI.

Happy Anniversary, HUBBLE!

Hubble Space Telescope launch.
Hubble Space Telescope on its way to orbit aboard space shuttle Discovery. Courtesy NASA.

It’s hard to believe that it’s been 30 years since the Hubble Space Telescope was launched into orbit on April 24, 1990. On the whole, they’ve been very good and productive years, despite the mission’s rocky beginning. Without it, our knowledge of the universe would be less advanced than it is today.

Following Hubble from the Beginning

HST has played a big role in my life, and I’ve followed it avidly through the decades. For several years, I was a student at the University of Colorado, working toward a graduate degree. During part of that time, I was also a member of the HST/Goddard High Resolution Spectrograph team led by friend and co-author John C. Brandt. I joined the group about a month before launch, although I’d been working for him for a couple of years on comet images for a big atlas we were producing. Working with HST data and proposals (as I hoped to do) was a big incentive to join his team. (I go into more detail about that job and my first impressions of HST in this entry from 2015. And, you can search out many other stories I’ve done here by typing “Hubble Space Telescope” in the search box.)

The day of launch was pretty exciting. I remember watching from home (since it happened in early morning). Then, we waited for the first-light images. Our team leader shared some concerns they were having with focusing the images. Eventually, through persistent questioning and investigation by such folks as Dr. Sandy Faber and others, the bad news came out: the telescope’s mirror had a problem called “spherical aberration”. It meant the main mirror was ground precisely wrong and that images would look incredibly fuzzy and out of focus.

galaxy M100 before and after Hubble Space Telescope was repaired
This comparison image of the core of M100 shows Hubble Space Telescope views before and after it was refurbished to correct for spherical aberration. Corrective optics inside the Wide Field and Planetary Camera 2 (WFPC-2) were able to sharpen the view. Courtesy NASA/ESA/STScI.

The news was devastating. We talked about what effect the spherical aberration would have on our instrument. It was not good. But, over time, as we all know, the HST teams were able to come up with ways to treat the images and data to pull out as much data as they could. And, eventually, the telescope started returning the “pretty pictures” that we all craved. It made my secret ambition to collect good images and information a bit easier.

Telling a Tale of Hubble Science

I began working on an article that then became a possible thesis topic, and eventually a book. Hubble Vision was published in 1995, just a few short years after launch and the first servicing mission. It was the first book to focus almost exclusively on HST science and it was written to share Hubble’s scientific achievements with the general public. My goal was to tell the tale of the telescope’s history, and then focus on the science story, not gossip and politics. I invited Jack to join me as the second author, and between us, we told a compelling tale of discovery. I’m still very proud of it.

Other writers made more money selling negative stories, but I felt good talking about the science. No matter how hard it was to get. I still write about HST science today, and it’s still cranking out good science. My most current book, The Discovery of the Universe, examines it as part of a family of space- and ground-based observatories that together continue our exploration of the cosmos.

Hubble’s Views of the Universe

I left the GHRS team when I graduated, and have since gone on to write about Hubble’s imagery and science many times in articles, books, and in this blog. Nothing the telescope sees fails to amaze me. Even the blobbiest-looking elliptical galaxy that HST shows us has a compelling story to tell. Throughout the 30 years of its mission, HST has studied the closest planets and the most distant objects in the observable universe. It taught us to see beyond our preconceptions of the cosmos, to learn that there are still new things to discover “out there.

Hubble’s First Deep Look

The first image that really took my breath away in Hubble’s early days was the very first Hubble Deep Field. This “core sample” of a tiny spot in the sky near the constellation Ursa Major, blew people away. I remember standing in front of it at a meeting of the American Astronomical Society in 1996, marveling at the detail.

Essentially, astronomers used Hubble to peer across billions of light-years, back to a time when the universe was very young. The Deep Field showed that galaxies exist as far as we could see. Some of them looked like shreds of galaxies, others looked fully formed.

Hubble Space Telescope first Deep Field image.
The first deep field image taken by Hubble Space Telescope. It revealed distant galaxies in the early universe. Courtesy NASA/ESA/STScI

The success of that image led to other deep field observations, in other directions of the universe. As far as we can tell, it’s galaxies (and their precursors) all the way out. And, today, thanks to HST, we have a much better idea of conditions in the early universe, back when the first stars and galaxies began to form.

That, to me, is one of the many incredibly enduring legacies that Hubble Space Telescope and the astronomers who’ve used it have created. I was pleased to be able to put it in the second edition of Hubble Vision. I also used later deep field images taken by the telescope in a very popular fulldome show about HST, now in its own second “edition”, called Hubble Vision 2.

Hail Hubble!

I encourage everybody to check out the many gorgeous images and news stories about the Hubble Space Telescope amassed by the folks at the Space Telescope Science Institute. They maintain a fantastic news site and have created a celebration page featuring links to great images, videos, and articles.

Help celebrate 30 years of remarkable achievements. Like everyone else who has ever met an obstacle and succeeded despite it, the Hubble Space Telescope and its science teams and astronomer-users have done the same. In the process, they have brought us new looks at the ever-changing universe.

Exploring Science and the Cosmos

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