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Human Exploration of the Cosmos: Paving the Way for Future Frontiers

The story of human exploration of the cosmos is one of curiosity, innovation, and boundless determination. From the early days of gazing at the stars to the current era of planning missions to distant planets, our journey into the cosmos has been both fascinating and consequential. The knowledge gained from past explorations has not only deepened our understanding of the universe but has also become the guiding light for the ambitious missions we aspire to undertake in the future.

The Pioneering Days:

Humanity’s fascination with the cosmos can be traced back to ancient civilizations, where early astronomers observed the night sky and developed intricate celestial maps. Fast forward to the space age in the mid-20th century, and we find ourselves witnessing the launch of the first artificial satellite, Sputnik 1, by the Soviet Union in 1957. This moment marked the beginning of human space exploration, opening up new frontiers beyond our home planet.

Moon Landings and Beyond:

The Apollo moon landings in the late 1960s and early 1970s represented a monumental leap for humankind. Astronauts ventured beyond Earth, setting foot on the lunar surface and capturing imaginations worldwide. The technological advancements and knowledge gained from these missions laid the groundwork for future space endeavours, serving as a testament to human ingenuity and determination.

Space Stations and Long-Term Habitation:

The construction and operation of space stations, such as the International Space Station (ISS), have allowed humans to live and work in space for extended periods. The ISS serves as a microgravity laboratory, offering insights into the effects of long-duration spaceflight on the human body and providing a platform for experiments that shape our understanding of fundamental scientific principles.

Rovers, Probes, and Robotic Exploration:

In addition to manned missions, robotic exploration has played a pivotal role in expanding our cosmic knowledge. Rovers like those on Mars, orbiters studying distant planets, and probes delving into the mysteries of comets and asteroids have provided invaluable data that informs our understanding of the solar system and beyond.

Toward the Future:

As we stand on the cusp of a new era of space exploration, lessons learned from past missions continue to guide our path forward. Ambitious plans include returning humans to the Moon, with the Artemis program aiming to establish a sustainable lunar presence. Beyond that, the prospect of crewed missions to Mars captures the imagination, fuelled by technological advancements and the lessons gleaned from decades of space exploration.

Innovation and Collaboration:

The quest to explore the cosmos is not only a testament to human curiosity but also a beacon for international collaboration and technological innovation. Partnerships between space agencies, private companies, and the scientific community propel us toward a future where humans may one day step foot on distant planets, opening up new possibilities for scientific discovery and the potential for life beyond Earth.

In conclusion, the human exploration of the cosmos has been a remarkable journey that continues to shape our understanding of the universe. The knowledge gained from past endeavours serves as a catalyst for future missions, inspiring us to reach new heights and fostering a collective dream of exploring the cosmos in ways previously unimaginable. As we look to the stars, the lessons of our cosmic past illuminate the path toward an exciting and promising cosmic future.

LeaningTower

School Holiday Adventures Await At The Gravity Discovery Centre & Observatory

School holidays are upon us, and at The Gravity Discovery Centre & Observatory, we have a mission: to make learning an unforgettable adventure for your children. As parents, you’re constantly on the lookout for engaging and educational activities, and we’ve got you covered. From rocketry to interstellar exploration and mesmerizing nights under the stars, here’s a glimpse of what’s in store for your little ones this holiday season.

Rocket Making Adventure (Wednesdays & Fridays): 

Imagine your child’s eyes lighting up as they design, build, and launch their very own rockets. Welcome to our “Rocket Making Program” during the school holidays on Wednesdays & Fridays! This hands-on workshop is a thrilling fusion of art and science. From crafting rocket bodies to decorating nose cones, creativity knows no bounds.

But the best part? The exhilarating rocket launch! Children will witness the power of science first hand as their homemade rockets soar into the sky, reaching for the stars. Along the way, they’ll grasp the intricacies of aerodynamics, physics, and propulsion. It’s more than an adventure; it’s an opportunity to ignite their curiosity about space exploration while having an absolute blast!

Space Explorers Expedition (Thursdays): 

On Thursdays in the holidays, let your young explorers embark on our “Space Explorers Program.”mThis program is a cosmic journey through our solar system, designed to captivate young minds and inspire a lifelong love for science.

Through interactive activities and captivating presentations, children will delve into the mysteries of our solar neighbourhood. From the scorching surface of Venus to the icy enigmas of Neptune, they’ll uncover the secrets of each celestial body. This isn’t just a journey; it’s an opportunity to nurture a deep appreciation for the vastness of space and the incredible diversity of celestial phenomena that exist beyond our world.

Observatory Tours and Stargazing (Throughout the Holidays) 

But the adventure doesn’t end there! Most nights during the school holidays, we invite you and your budding astronomers to our Observatory Tours. Venture to our observatory, where the wonders of stargazing come to life. It’s a chance for your family to explore the cosmos together.

Gaze upon distant galaxies, observe the delightful Saturn and its rings, and delve into the mysteries of the night sky. Our expert astronomers will be your guides on this celestial journey, ensuring you get the most out of this enchanting experience. It’s an opportunity to witness the wonders of the universe up close and personal, creating memories that will last a lifetime.

Secure Your Family’s Cosmic Adventure! 🚀🌌

At The Gravity Discovery Centre, we believe that learning should be an adventure. Our school holiday programs offer a unique blend of fun and education, promising your child unforgettable memories and a newfound passion for the marvels of science and space exploration.

Spaces are limited, so be sure to secure your family’s spot today. Join us for an out-of-this-world experience that unlocks the universe this school holiday season. Contact us at bookings@gravitycentre.com.au or call 08 9575 7577 to learn more and reserve your place in these exciting programs.

We can’t wait to show you the universe!

Wildflower Season Blooms at the Gravity Discovery Centre

It’s that time of the year again – wildflower season at the Gravity Discovery Centre is bursting with colour and life. If you’re into nature, Insta-worthy shots, or just curious about what’s blooming, we’ve got you covered.

Highlighting a few blossoms of the season:

1. Caladenia longicauda – The White Spider Orchid is notable for its long, slender sepals and petals, which give it a distinct spider-like appearance.
2. Pterostylis vittata – The Banded Greenhood is an evergreen terrestrial orchid, unique because it does not produce nectar but instead attracts pollinators through its appearance.
3. Caladenia flava – Known as the Cowslip Orchid, this species is recognized by its bright yellow flowers with red markings. It’s a favourite among native bees for pollination.
4. Pterostylis dilatata – The Green Snail Orchid is fascinating in its growth pattern, often emerging after bushfires, signifying nature’s resilience.
5. Pterostylis arbuscula – The Dwarf Greenhood gets its name from its small stature, often growing to a height of only about 10 cm.
6. Kennedia prostrata – The Running Postman is a sprawling ground cover plant. Its name is derived from its vibrant red flowers resembling the red coats of early British postmen.
7. Philotheca spicata – The Waxflower has oil glands in its petals which make them glisten, giving it its wax-like appearance.
8. Lysinema ciliatum – The Curry Flower stands out due to its fringed petal edges, providing a soft, feathery appearance.

In the coming days, the Elythranthera brunonis or the Purple Enamel Orchid is expected to bloom, definitely a fan favourite here at the centre.
Oh, and did we mention the family of Drosera? We’ve identified 7 unique species here. Commonly called sundews, these intriguing plants are not just beautiful but also carnivorous!

Why is this important? 🌍

Western Australia is a biodiversity hotspot. This means it’s home to a variety of plants and animals that you won’t find anywhere else in the world. Biodiversity (a combination of the words ‘biological’ and ‘diversity’) refers to the variety of different species inside an ecosystem. The array of wildflowers is not only a visual feast but a reminder of our responsibility to safeguard the balance of our ecosystems. If you’re planning a visit and have questions or are keen to spot these floral gems, do approach one of our astronomers Mitch. Whilst at night his head is in the stars, by day he
looks down at the ground beneath us to take in all of nature’s wonders no matter how big or small.

Pull out your cameras, bring your buddies and immerse yourself in nature’s playlist.

Asteroids: Exploring the Intriguing Cosmic Nomads

In the vast expanse of our solar system, an array of celestial objects dance around the sun, each with its own unique story to tell. Among these captivating entities, asteroids stand out as fascinating and enigmatic cosmic wanderers. In this article, we delve into the world of asteroids, uncovering their origins, characteristics, and the pivotal role they play in shaping the cosmic landscape.

Asteroids are rocky, airless remnants that populate the space between planets in our solar system. Often referred to as “minor planets” or “planetesimals,” these fragments hold vital clues about the early days of our solar system and the processes that led to its formation.

Asteroids are thought to be leftover building blocks from the formation of planets, a remnant of the solar system’s birth approximately 4.6 billion years ago. They vary in size from small pebbles to massive bodies, with some even exceeding hundreds of kilometres in diameter.

Most asteroids are composed primarily of rock and metal, resembling miniature planets that never coalesced into a larger whole. Some, known as carbonaceous asteroids, contain higher levels of carbon and water-bearing compounds, making them intriguing targets for scientists searching for the building blocks of life.

Asteroids are categorized into different classes based on their characteristics and composition. The three primary categories are:

  1. C-Type (Carbonaceous) Asteroids: These are the most common type and are rich in carbon compounds. They are often found in the outer asteroid belt and are believed to be among the oldest objects in the solar system.
  2. S-Type (Silicaceous) Asteroids: These asteroids are composed mainly of silicate materials and metals. They are typically found in the inner asteroid belt and represent a more diverse group in terms of composition.
  3. M-Type (Metallic) Asteroids: These asteroids are rich in metals, such as nickel and iron. They are often found in the middle of the asteroid belt and may be fragments of larger bodies that underwent significant differentiation.

Asteroids follow elliptical orbits around the sun, and their trajectories can bring them in close proximity to Earth. While the vast majority pose no immediate threat, the potential impact of a sizable asteroid remains a topic of concern for scientists and astronomers.

Notable incidents, such as the Tunguska event in 1908 and the Chelyabinsk meteor in 2013, underscore the importance of tracking and understanding the movements of asteroids that cross Earth’s orbit. Organizations like NASA actively monitor near-Earth objects and work on strategies to mitigate potential impacts.

Studying asteroids provides valuable insights into the formation and evolution of the solar system. By analysing their composition, scientists can uncover clues about the conditions that prevailed during the early stages of our cosmic neighbourhood’s development. Asteroids may also hold answers to questions about the origins of water and the building blocks of life on Earth.

Asteroids are more than just celestial oddities; they are time capsules that offer a glimpse into the past and the dynamic processes that have shaped our solar system. As we continue to explore and learn about these ancient relics, we unlock a deeper understanding of our cosmic origins and the intricate interplay that has shaped the universe we call home.

Image credit: NASA

The jets of Enceladus

Credits: NASA, ESA, CSA, STScI, and G. Villanueva (NASA’s Goddard Space Flight Center). Image Processing: A. Pagan (STScI).

NEW JAMES WEBB IMAGE ALERT!…….and this one is cool!

The James Webb space telescope has recently taken a photo of Saturn’s icy moon Enceladus, the image can be viewed above and shows up as a white pixel in the image (highlighted in red). The moon itself in this image is not exciting; however, pictured below the white pixel (the moon), you can see jets of material coming off the moon. That substance is water, which is being ejected over 9,000kms!!

And… it’s feeding into the rings of Saturn!

Water being ejected off the surface of this moon is not a new discovery, that discovery was made quite dramatically in 2005 when the Cassini space probe pictured them erupting from the surface of the moon on one of its flybys. In fact, Enceladus is not the only moon to do this, Jupiter’s Icy moon Europa along with a few others has this same feature, which is water jets shooting off its surface. What is a discovery based on this image is just how far those plumes of water (also called geysers) reach into space, originally believed to reach several hundred km out, this new photo has given NASA a distance of over 9,000 km that the water jets reach out to, this is because the moon has little to no atmosphere and any thick atmosphere that does start to form doesn’t last for long due its weak gravity unable to hold onto it, the gravity is also weak enough that the pressure from the water jets can overcome it to reach those heights! 
This process of shooting water plumes off its surface is called cryovolcanism, “cryo” meaning cold and in this case, water vapor or Icey particles.
Above image is of Saturn’s moon Enceladus with the water plumes erupting from its south pole, taken by the Cassini space craft. Image Credit: NASA/JPL/Space Science Institute
This illustration shows NASA’s Cassini spacecraft diving through the plume of Saturn’s moon Enceladus, in 2015. Image Credit: NASA/JPL-Caltech
Life in the moons?
The biggest detail of these water plumes or jets is the fact that they have evidence that life could be present under the icy surface of this moon. The moon’s surface is completely covered by ice, after all, it is around -200℃ out there, however, under all that ice are oceans of salty water, heated to liquid by heat due to the tidal forces exerted on it from Jupiter and the other big moons.

Scientists believe life may have originated deep underwater where heat makes its way up from the Earth’s hot core through openings called hydrothermal vents, heating the water to help provide conditions to support life through chemical energy and food rather than energy from the Sun. (see picture graphic below for visuals).
Scientists believe that hydrothermal vents present on moons such as Enceladus could also help spur life on within its waters.
Also, the Cassini spacecraft flew directly through one of these plumes of water during one of its flybys and its sensors detected organic compounds. Now, this isn’t to say without a doubt life is present within its waters, but some of the ingredients are there!

Ok, so it won’t be any forms of intelligent life, however, any other life form outside of Earth would be a big find! It would confirm that the universe can easily make life outside of Earth and help to support the idea that life began here on Earth due to that process. As it stands the origins of life are still somewhat of a mystery.

Everyone looks to planets in search of life when actually the moons are the biggest bet to find it (within our solar system anyway).
Photo Credit: Southwest Research Institute
For anyone interested in more reading, here is the link to NASA’s Webb image and story, including how it feeds into the rings of Saturn! 
Webb Maps Large Plume Jetting From Saturn’s Moon Enceladus | NASA

Bringing the Total Solar Eclipse to WA and the World

The Grand Eclipse Expedition of 2023

by

Richard (Rick) Tonello

Chief Astronomer GDC Observatory

 

On the 20th April 2023, along the sun drenched coastline of the Cape Range National Park, the Solar System will put on a spectacular show that will attract tens of thousands of people from across Australia and the world.

This celestial event will showcase the precision clockwork of the Solar System as the Sun, Moon and Earth perfectly align to create the spectacular phenomenon known as a Total Solar Eclipse.

Starting in the Great Southern Ocean, the shadow of the Moon will race across the surface of Earth at over 2700Km/h, skim over the Exmouth Peninsula and race northward from the Australian continent toward Timor-Leste and the Pacific Ocean.

For people along the narrow “Line of Totality” they will witness the Moon completely cover the blinding disc of the Sun revealing the complex structure of the Solar Corona. For a brief 62 seconds, observers will be plunged into an eerie twilight and the sky looking like a bullet has pierced its familiar continuum.

While there is a Total Solar Eclipse every 18 months somewhere around the world, this eclipse is special. The 2023 event is a rare Hybrid Eclipse that occurs once every decade. A Hybrid Eclipse is where the distance between the Earth and Moon is so finely balanced, that the curvature of Earth influences how much of the Moon covers the disc of the Sun. From the starting point in the Great Southern Ocean any observers will see an Annular Solar Eclipse, from Exmouth observers will see a Total Solar Eclipse.

Astronomers from the Gravity Discovery Centre Observatory will be on an expedition to Exmouth to observe, photograph and live stream the entire Total Solar Eclipse from the line of totality.

Live images will be provided from two, specialised Solar Telescopes and high-resolution cameras. One telescope will observe the Photosphere (Light Sphere), the surface of the Sun, while the other telescope will observe the Chromosphere (Colour Sphere), the dynamic layer located above the photosphere.

The broadcast provided by the GDC Total Solar Eclipse Expedition will be broadcasted to their FaceBook Page and YouTube Channel.

Local Media, social media and other organisations will pick up the GDC Observatory Total Solar Eclipse broadcast on the day of the Eclipse. Organisations such as Tourism WA, the Museum of Western Australia, the Singapore Science Centre, and to the Yagan Square Multimedia Screen are just a few of the organisations to utilise the live stream.

 

Those who are not observing from the Path of Totality will observe a Partial Solar Eclipse. Depending on the distance of the Observer from the path of Totality, the less of the Sun’s blinding disc will be obscured by the Moon.

 

Observers from Perth will witness a little over 70% of the Sun’s disc obscured by the Moon. Even though a majority of the Sun’s disc is covered, it is still dangerous to observe without the proper eye protection.  Never look directly at the Sun, even during the Partially Eclipsed phases. Even a 99% obscured Sun is enough to cause Solar Retinopathy (irreversible eye damage). Always use approved Solar Viewing Equipment (Eclipse Glasses) with the ISO 12312-2:2015 markings.

 

There are many ways to enjoy the Partial Eclipse through indirect viewing such as Pin-hole cameras, Camera Obscuras, kitchen colanders and Live streaming services.

 

There are many sources of information regarding Safe techniques to observe the Total and Partial Solar Eclipse such as the NASA, Gravity Discovery Centre & Observatory and Astronomical Society of Australia websites.

 

Through public education and correct information, let’s make this a date to remember for all the right reasons.

 

A slow transient Magnetar has been found with the MWA

Ok so my suggestion to name this object LGM (Little Green Men) 2 was declined by my team Haha but we still aren’t 100% sure that these objects are Magnetars, and to avoid any potential conspiracy addicts (if you’re reading this) going into overdrive right now, it’s not aliens, my LGM 2 reference is a joke and ode to the original (half-jokingly name) LGM 1 which was given to the first Pulsar signal discovered before they knew it was a pulsar.

My Research team at CIRA (Curtin Institute of Radio Astronomy) has found a mysterious signal in Space, it is what we call a slow transient, transient meaning it turns off and on and slow meaning well… it does this slowly.

This signal was actually recorded in 2018 by the MWA Telescope but not discovered until 2021 when an Honours student-led by Curtin Astrophysicist “Natashia Hurley-Walker” was combing through old Archive records and stumbled upon this mystery signal. It turns on for 1 minute and then off for just over 18 minutes which would indicate it rotates once every 18 minutes and that’s odd, Reasons for which I’ll explain further in the article. The team has spent over a year since following up with further observations with the MWA, Parks Telescope in NSW, and NASA’s Chandra X-ray Observatory but here’s the kicker, the signal was only active for 3 months between February – March 2018 and has since turned off and hasn’t been detected since.

The team has also tirelessly looked through the last 10 years of observations from the MWA looking for this signal but to no avail, so it randomly turned on for what seems to be the first time in February 2018 and turned off a few months after and hasn’t been seen since. Weird!

 

This is an image of our Galaxy in radio light with the position of the discovered object highlighted. Credit: ICRAR.

 

So, then what’s a Magnetar? A Magnetar is a Neutron star! These objects are the leftover collapsed dense cores of giant stars after the star explodes in a supernova! The core itself is mainly all Neutrons packed tightly into a ball with some Protons and Electrons in there that survived the collapse. Stars are already spinning, but when the star explodes and its core collapses, this causes it to spin faster and faster as it gets smaller, this is due to the conservation of angular momentum (think of a figure skater spinning on ice, they speed up as they draw in their arms).
This also makes the magnetic field skyrocket up in strength to a billion times stronger than our own Sun’s magnetic field! That’s strong enough to erase your credit card from a 100,000Km away! Magnetars are the most magnetic objects in our universe.
These Neutron stars are Dense, which means they have terrifyingly strong gravity! A single cubic Cementer of Neutronium (which is what Neutron stars are made up of) would outweigh Mount Everest!

Now only around 10% of all neutron stars turn into Magnetars, there is also another type of Neutron star that spins fast and as they spin, they produce beams of energy (Light) out of their North and South Magnetic poles, these objects are called Pulsars! These dead stars spin and as they spin, these beams of light turn with it (think of a lighthouse) when the beam of light turns and flashes at the earth, we see this pulse of light and can detect them via Radio Telescopes, but although rarer, Magnetars can also produce these Beams!
So, recap, all Pulsars and Magnetars are simply Neutron stars but with added more unusual properties!

What’s most important now is that we are not 100% sure what causes these Neutron stars to produce these emission beams. We do know that it’s to do with their strong magnetic field coupled with their fast spin that accelerates electrons on their surface & above its surface up the open magnetic field lines and well that’s what makes this discovery weird! At a spin of 18 Minutes per hour, that’s insanely slow for these objects and as far as our understanding goes, this just isn’t fast enough to produce the beams that we are detecting!

The first thing we were able to determine was it seems to be within our own Galaxy. Its Dispersion Measure (DM) is around 56 and so we can then calculate its rough distance using a model called the electron distribution model to find a distance of 1.3Kpc (kiloparsec) which is well within our own galaxy.

Why do we think it’s a Magnetar? well, that’s tricky to explain but we take all the data and measurements from the radio light it has emitted and deduced many aspects of its characteristics which all seem to match that of Magnetars and Pulsars, such as its Polarization angle and how it flattens across each Pulse, it’s Spectral index, most pulsars/Magnetars show a systematic increase in pulse width and separation of profile components when observed at lower frequencies (meaning emissions at higher frequencies are being produced closer to the surface of the neutron star than at lower frequencies), also it’s around 90% Linearly polarized which all Pulsars and Magnetars generally are and along with other things which unless you want a 10-page article ill avoid going into for now.

I should now add that we have found a second slow transient which we believe to be another Magnetar, however, this one has a rotational period of 22 minutes (even slower) and has been active for the last 5 or 6 years after following up previous data from the MeerKAT Telescope in South Africa, how did that one go undiscovered for so long? it’s got very similar properties to the first discovered object, i.e., angle of polarization and pulse flattening however its Spectral index appears to be different along with other characteristics that could suggest it’s a completely different object.

this all leads to bigger questions, have we just discovered two of the same Objects, and in which case how they have not got picked up previously?
Or have we discovered two completely different objects? which seems even more absurd!

We are working behind the scenes to unravel this mystery, do more follow-ups, and look for other objects emitting slow pulses that fit the same profile… STAY TUNED!
Here is also a quick article you can read on two Neutron stars colliding creating what we call a Kilonova….COOOOOOL! Thanks to Mitch for finding and sending through! Mitch is one of our amazing Astronomers here at the GDC!
If you want to learn more about how these types of objects are created or to understand fully, then you really need to know the full cycle of how stars live their lives and die! what makes some stars fuse heavier elements? what determines if those big stars turn into Neutron stars or black holes? If this interests you, then I’d highly recommend coming to our advanced talk on the Life and Death of Stars! We won’t hold back on the physics so come along, sit down and you might want to strap yourself in! 

You can book here, and you won’t be disappointed! The night includes looking at some of these objects through our telescopes!

And as always if you have any questions then feel free to send me an email here and I’ll happily answer them and feature your question in our article next Month!

Until then keep looking up!

The Neergabby Star Party Timetable of Events 2023

 

Neergabby Star Party Timetable of Events

The Gravity Discovery Centre & Observatory along with the Shire of Gingin presents the Neergabby Star Party.

Program:

DayTimeSession Detail
Friday 17th March2pm-6pmCheck-in at Neergabby grounds, park-up, set up camp and telescopes
5pm-7pmSausage sizzle available for purchase
7pm – 8pmCultural storytelling
8pm-10pmPublic stargazing run by the GDC at the Neergabby grounds/Amateur astronomer observing and astrophotography (can continue past 10pm)
Saturday 18th March10am-4pmDaytime activities at the Gravity Discovery Centre (additional cost)Activities include: Presentations by GDC astronomers and special guests, Solar observing and tours of the ZADKO research observatory.

To purchase a daytime ticket (includes activities) for the Gravity Discovery Centre click here.

5pm-7pmSausage sizzle available for purchase
8pm-10pmPublic stargazing run by the GDC at the Neergabby grounds/Amateur astronomer observing and astrophotography (can continue past 10pm)
Sunday 29th May10amCamping check out

Comet C/2022 E3 (ZTF) What do we know and how can you see it?

Comet C/2022 E3 (ZTF) is a newly discovered comet that was first observed in 2022 by the Zwicky Transient Facility (ZTF), a survey aimed at capturing transient astronomical events. It is named after the facility and its discovery year, 2022. Astronomers believe the Comet last visited us some 50,000 years ago. It has been nicknamed “The Green Comet” because of the out-gassing and ionisation of diatomic-Carbon along with cyanogens. Comets are small, icy bodies that originate in the outer solar system and can become visible when they approach the sun and release gas and dust, creating a glowing tail. The exact characteristics and behavior of C/2022 E3 (ZTF) are not known, but it is being monitored by astronomers to gather more information.

The Comet will be visible to us in the Southern Hemisphere in early February. To observe the Comet you will need a dark sky, a clear view to the North and either a pair of binoculars or a telescope. The best nights to view the comet will be Thursday 9th February, Friday 10th of February and Saturday 11th February with Saturday 11th being the best night overall. If you do try and view the Comet any earlier than these dates you will have to contend with the brightness of the Moon which will affect visibility.
The Gravity Discovery Centre & Observatory not only has a clear Northern aspect, but large telescopes in a world class Observatory under dark skies, with passionate astronomers ready to show you the Green Comet of 2023 (along with other incredible targets).
 
On Friday 10th & Saturday 11th of February, the GDC Observatory will be hosting two Comet Sessions to observe Comet C/2022 E3 (ZTF) along with a pre-tour presentation (about comets) so you can learn all about these “Hairy Stars” that grace our skies every now and then. If you would like to make a booking for the Comet session click here and book the Observatory tour on either 10th or 11th of February.
 
On Saturday the 11th Feb, Chief Astronomer Rick, will be doing a Live-Sky broadcast from a “Super-Secret” location when Comet C/2022 E3 (ZTF) will be located just above the planet Mars.
 
Book your tickets now for our special Comet Observing Sessions at the GDC Observatory or tune into our FaceBook page on Saturday 11th February at 8:30pm for a Live-Sky Astronomy “Comet Special.”
Disclaimer: We’re not sure how bright The Green Comet will be. Comets are fickle things, they may become bright enough to observe with the naked eye, or they may be really faint.
Either way, if you get out there with your binoculars or scope, you’re still going to have a lot of fun, or join us at the GDC Observatory and observe this “Hairy Star” from our telescopes.