Articles Archive - /en-eu/blog/ The Telescope Reinvented Wed, 01 Jul 2026 08:31:41 +0000 en-EN hourly 1 https://wordpress.org/?v=6.8.6 /wp-content/uploads/2023/12/cropped-unistellar-favicon-2-32x32.png Articles Archive - /en-eu/blog/ 32 32 3 Reasons to observe this month /en-eu/blog/3-reasons-to-observe-this-month/ Wed, 01 Jul 2026 06:00:00 +0000 /blog/3-reasons-to-observe-this-month/ Every month, discover three unmissable celestial events to observe with your Unistellar telescope.

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The Summer Triangle

 

In the August sky, a distinctive geometric figure can help you find your bearings: the Summer Triangle.

 

Easily recognizable to the naked eye, this asterism connects three of the sky’s brightest stars: Vega, Deneb, and Altair.
A few suggestions to explore in this region with your telescope:

 

The Veil Nebula, in the constellation Cygnus: a vast structure, remnant of a supernova. Several segments are particularly striking, including NGC 6992 and NGC 6960.

The Snowball Nebula (NGC 7662), in the constellation Aquila: a more subtle target that becomes visible after about 10 minutes of observation.

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M11: a star cluster in the Scutum Star Cloud

 

M11, the Wild Duck Cluster, is an exceptionally rich open cluster situated on the northern edge of the Scutum Star Cloud, in the summer Milky Way. More than 6,000 light-years away, several thousand tightly packed stars give the impression of a compact, luminous cloud; through a telescope, this ‘pseudo-globular cluster’ resolves into a multitude of bright points, offering a spectacular view from the very first minutes of observation.

 

M1 Crab Nebula

M11 : Photo Credit Stuart Fort

NGC 6946 – The Fireworks Galaxy

 

Between the constellations of Cygnus and Cepheus lies NGC 6946, a spiral galaxy nicknamed the “Fireworks Galaxy.”
In just a century, it has hosted ten supernovae (exploding stars at the end of their life) visible from Earth, an absolute record!

 

Its twisted arms, reddish hues, and star-forming regions make it a fascinating but faint target: your telescope will need a bit of time to fully reveal its structure.

Fireworks Galaxy (NGC 6946)

NGC 6946 : Photo Credit Stuart Fort

See you next month for more reasons to look up!

Happy stargazing with .

Further readings

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Two spooky appearances in the sky for Halloween /en-eu/blog/two-spooky-appearances-in-the-sky-for-halloween/ Mon, 27 Oct 2025 19:27:47 +0000 /?post_type=blog&p=284090 Every month, discover three unmissable celestial events to observe with your Unistellar telescope.

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Two frightening celestial objects incoming this Halloween : the Eastern Veil Nebula and the Wizard nebula

As autumn settles over the northern hemisphere, the night sky reveals two of its most elusive wonders that seem to whisper. This season, grab your telescope and let your gaze drift toward the constellations of ⲵԳܲ and Cepheus. There, two celestial shadows await : The Eastern Veil Nebula (NGC 6992) and the Wizard nebula (NGC 7380).

The Blood Veil of a Cosmic Widow : the Eastern Veil Nebula

 

The Eastern Veil Nebula takes on the appearance of a cosmic wound, a trail of blood suspended in the sidereal darkness. Born from the death of a star some 5,000 years ago, this glowing cloud stretches across the Cygnus constellation like the still-fresh scar of a stellar explosion. Part of a vast complex known as the Cygnus Loop, it lies alongside the Witch’s Broom and Bat Nebulae, weaving a tapestry of celestial horror in the void, where beauty and destruction merge.

Eastern Veil Nebula : Photo Credit Derrick Pearce

The Wizard nebula : The announcement of a spell that must be uncovered

 

To the naked eye, the region of Cepheus appears calm and unremarkable. But through a telescope, a spectral form emerges : the Wizard Nebula (NGC 7380). Shaped like a silhouette in a sorcerer’s robe casting a spell, this vast cloud of gas and dust seems to glow with an otherworldly glow. 7,200 light-years away, the nebula is a cradle of newborn stars whose radiation sculpts its ghostly pillars and folds

 

Both disturbing and mesmerizing, the Witch Star Nebula seems to float between darkness and flames… a cosmic apparition frozen in motion. This magical spectacle, perfectly suited to the Halloween sky, is best seen on clear autumn nights.

NGC 7380: Photo Credit Greg Warwick

Tips for Observation

 

  • Best time: October through November, when Cygnus and Cepheus are high in the evening sky.
  • Duration : Observe for 20 minutes to allow time for the telescope to collect enough light signal for these especially faint objects.
  • Equipment : Unistellar telescopes are perfect for this.

As you trace your telescope across the sky this autumn, pause on these scary objects. The Eastern Veil Nebula and the Wizard Nebula remind us that some figures hide quietly among the stars, waiting for those who take the time to watch.

 

Clear skies, and happy observing.

Happy stargazing with .

Further readings

The post When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope appeared first on .

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3 Reasons to observe this month Halloween Edition /en-eu/blog/3-reasons-to-observe-this-month-halloween-edition/ Fri, 24 Oct 2025 07:35:29 +0000 /blog/3-reasons-to-observe-this-month-halloween-edition/ Every month, discover three unmissable celestial events to observe with your Unistellar telescope.

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In October, night falls earlier, mists begin to rise, and the stars seem to multiply. It’s the month when imagination blends with science—when every point of light becomes a cosmic mystery.


For Halloween, the sky turns into a strange scene: silhouettes of sorcerers, stellar ghosts, and magical spheres hide among the stars… and it’s up to you to help us uncover them.


To inspire you, we’ve observed three intriguing celestial objects that herald the imminent arrival of Halloween:

The Face of a Wizard – NGC 7380

 

Lost within the constellation of Cepheus, NGC 7380—nicknamed the Wizard Nebula—seems to have stepped straight out of an ancient tale.
Its structure of gas and dust, sculpted by stellar winds, reveals a mysterious profile: a brow, a nose, a beard… almost human.


Born only a few million years ago, this nebula is still in turmoil: young stars are forming within it, their radiation lighting up the surrounding cloud. Under a clear autumn sky, it offers a striking sight — a celestial wizard frozen in light.

 

NGC 7380: Photo Credit Stuart Fort

The Ghost of Mirach – NGC 404

 

In the constellation of Andromeda, just a few arcminutes away from the bright star Mirach, hides a small galaxy almost invisible to the naked eye.


Its faint light seems to overlap that of its dazzling neighbor, creating the illusion of a spectral presence — hence its haunting nickname, the Ghost of Mirach.


This elliptical galaxy lies about 10 million light-years away. There’s nothing truly frightening about it, but observing it is a challenge: one must carefully separate it from Mirach’s bright halo. When you succeed, it feels like uncovering a hidden secret — a ghost concealed behind a star.

 

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NGC 404: Photo Credit Pierre Auchatraire

The Bubble Nebula – NGC 7635

 

Let’s head to Cassiopeia to admire one of the most beautiful structures in the deep sky: the Bubble Nebula (NGC 7635).


At first glance, it looks like a perfect sphere suspended in space — a cosmic bubble inflated by the fierce winds of a massive star.


But in the dim light of October, it’s hard not to see it as a magical orb, a glowing spell floating among the stars.

This bubble of gas, seven light-years across, continues to slowly expand into the interstellar void. Its bluish outline, highlighted by the surrounding gases, evokes a sleeping spirit or a breath of energy ready to fade away.

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Bubble Nebula: Photo Credit Yann-Michel Niquet

Now it’s your turn to observe — grab your telescopes and join us in this celestial hunt before Halloween!


In our next Newsletter, the best observations will be featured (with your permission).

4. Bonus: Eclipses on Jupiter

Happy stargazing with .

Further readings

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Titan’s shadows /en-eu/blog/titan-shadows/ Mon, 07 Jul 2025 09:15:23 +0000 /?post_type=blog&p=280764 Every month, discover three unmissable celestial events to observe with your Unistellar telescope.

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Witnessing Saturn’s Cosmic Ballet: A Summer of Transient Events

 

This summer, the ringed planet Saturn takes center stage in our night sky, offering amateur astronomers a rare opportunity to observe fascinating transient events. Among these celestial spectacles, the shadow transits of Titan, Saturn’s largest moon, promise to be particularly captivating. Just as we previously explored Jupiter’s moon eclipses, these Saturnian events provide a dynamic viewing experience that changes from night to night.

Moon Titan appears in front of Saturn in an image captured by NASA’s Cassini spacecraft. Credit: NASA/JPL-Caltech/Space Science Institute

Upcoming Titan shadow transits in Universal Time (GMT)

 

Date

Start

Mid-transit

End

May 15

9:49

12:59

15:44

May 31

9:05

12:12

14:53

June 16

8:21

11:24

14:00

July 2

7:40

10:35

13:03

July 18

7:00

9:44

12:05

Aug. 3

6:25

8:52

11:04

Aug. 19

5:52

8:01

10:00

Sept. 4

5:25

7:09

8:50

Sept. 20

5:09

6:20

7:34

Oct. 6

5:32*

Start and end times are when Titan’s full shadow is first and last visible entering and exiting Saturn’s disk, respectively. * Full shadow on disk only at mid-transit (source: Sky and Telescopes)

The Science Behind the Spectacle

 

These shadow transits occur because of the unique alignment of Saturn, its rings, and its moons from our vantage point on Earth. As Saturn progresses on its 29.5-year orbit around the Sun, our angle of view changes, sometimes showing the rings head-on (as in 2018 or 2033) and sometimes making them virtually disappear, as in 2025 or 2040, when the Earth is lying in the plane of the rings and moons. During these aligned periods, we can observe moons and their shadows crossing the planet’s face. So it’s either now or in 15 years!

Titan’s shadow is particularly noticeable because of the moon’s size – at 5,150 km in diameter, it’s larger than Mercury and second only to Jupiter’s Ganymede in our solar system. When Titan passes between Saturn and the Sun (from our perspective), its substantial size creates a clearly visible shadow on Saturn’s cloud tops.

As you turn your telescope toward Saturn this summer, remember that you’re witnessing a cosmic dance that has been playing out for billions of years. Each transit offers a unique opportunity to connect with the mechanics of our solar system and appreciate the beauty of celestial motion.

Happy observing!

Further readings

The post When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope appeared first on .

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Unistellar Community Included In Multiple Scientific Papers /en-eu/blog/unistellar-citizen-astronomers-included-in-multiple-scientific-papers/ Tue, 27 Feb 2024 14:49:01 +0000 /blog/unistellar-citizen-astronomers-included-in-multiple-scientific-papers/ Did you know Unistellar Citizen Astronomers are often cited in published scientific papers? Find out how you can contribute too!

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Getting a paper published in a scientific journal is a major achievement for any scientist, giving them the chance to share the new discoveries they’ve made. But you don’t need to have a fancy degree or work at a university to make scientific discoveries. With the right tools, anyone can contribute to science.

In just the past few years, Unistellar Citizen Astronomers have been recognized in multiple scientific publications on exoplanets, space missions and more. That comes thanks to the partnership between Unistellar and the SETI Institute, which gives astronomers access to Unistellar Network data for their research. As research grows in scope, astronomers simply don’t have the resources to make all the observations they need to understand our universe. That’s where Unistellar Network members come in.

A map of member locations around the globe.

Our network is a worldwide community of Citizen Astronomers who use their Unistellar telescopes to collect astronomical data. Collaborating over social media and the messaging platform Slack, observers from different countries strategize ways to gather the best data on asteroids, comets, exoplanets and more. Recent successes include refining the shape of the Lucy mission target asteroid Eurybates and a record-breaking observation of the exoplanet Kepler-167 e.

Future observations can help astronomers discover new exoplanets, get better data on the size and orbit of potentially hazardous Near-Earth Asteroids, and keep an eye on ongoing space missions. Unistellar has lots of resources for Citizen Astronomers – plus, the ease-of-use of the Unistellar telescopes and dedicated app make doing Citizen Astronomy fun and approachable for anyone.

“With the Unistellar Citizen Astronomy community, there is always something new and fun to look at,” says Unistellar Citizen Astronomer Georges Simard in Quebec. “It is an incredible and easy way to learn about astronomy and contribute to real research projects.”

To learn more, check out our index of scientific publications featuring Unistellar Network contributions:

Index of Scientific Publications

Peer-Reviewed Articles

  • Sicardy, B., et al., Constraints on Trito atmospheric evolution from occultations: 1989-2022, A&A, in press, 2024 https://arxiv.org/abs/2402.02476

  • Graykowski, A. et al., Faint Comet Detection with Unistellar eVscopes, Research Notes of the AAS, Volume 8, Issue 2, id.41. , 2024 https://iopscience.iop.org/article/10.3847/2515-5172/ad25f9

  • Pereira, C. L. et al., the two Rings of (50000) Quaoar, A&A, 673 L4, 14, 2023

  • Graykowski, A. et al., Light Curves and Colours of the Ejecta from Dimorphos after the DART impact, Nature 6161, 5957, 461-464, 2023 https://www.nature.com/articles/s41586-023-05852-9

  • Yoshida, F. et al., Multi-chord observation of stellar occultation by the near-Earth asteroid (3200) Phaethon on October 3, 2021 (UTC) with very high accuracy, Publication of the Astronomical Society of Japan, 75, 1, 2023 https://academic.oup.com/pasj/article/75/1/153/6947807
  • Lambert, R. et al., Rotation Period Determination for (7335) 1989JA, Minor Planet Bulletin, 50,1, 16-17, 2023 https://articles.adsabs.harvard.edu/full/2023MPBu…50…16L
  • Peluso, D. O., et al., The Unistellar Exoplanet Campaign: Citizen Science Results and Inherent Education Opportunities, Publications of the Astronomical Society of the Pacific, 2135, 1043, 2023 https://www.nature.com/articles/s41586-023-05852-9
  • Perrocheau, A., A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network. The Astrophysical Journal Letters940.2 (2022): L39.
  • Cazeneuve, D., et al., ODNET, The Astrophysical Journal, 165, 1, 11, 2023 https://articles.adsabs.harvard.edu/full/2023MPBu…50…16L
  • Sibbernsen, K. 2022. Electronic telescopes and their use in astronomy education. The Physics Teacher, 60(5), 394.
  • Barbosa, D., Coelho, B., Bergano, M., Magalhães, C., Mendonça, D., Silva, D., Correia, A.C. M., Pandeirada, J., Ribeiro, V., Esposito, T., Marchis, F., 2022. Cyber-Cosmos: A new citizen science concept in a dark sky destination. Acta Astronaut. 200, 612–619.
  • Pearson, K.A., Beichman, C., Fulton, B.J., Esposito, T.M., Zellem, R.T., Ciardi, D.R., Rolfness, J., Engelke, J., Fatahi, T., Zimmerman-Brachman, R., Avsar, A., Bhalerao Varun, D., Boyce, P., Bretton, M., Burnett, A.D., Burt, J., Fowler, M., Gallego, D., Gomez, E., Guillet, B., Hilburn, J., Jongen, Y., Kataria, T., Kokori, A., Kumar, H., Kuossari, P., Lekkas, G., Marchini, A., Meneghelli, N., Ngeow, C.-C., Primm, M., Samantaray, S., Shimizu, M., Silvis, G., Sienkiewicz, F., Swain, V., Tan, J., Tock, K., Wagner, K., Wünsche, A., 2022. Utilizing a global network of telescopes to update the ephemeris for the highly eccentric planet HD 80606 b and to ensure the efficient scheduling of JWST. The Astronomical Journal 164.5 (2022): 178.
  • Wang, X.-Y., Rice, M., Wang, S., Pu, B., Stefánsson, G., Mahadevan, S., Radzom, B., Giacalone, S., Wu, Z.-Y., Esposito, T.M., Dalba, P.A., Avsar, A., Holden, B., Skiff, B., Polakis, T., Voeller, K., Logsdon, S.E., Klusmeyer, J., Schweiker, H., Wu, D.-H., Beard, C., Dai, F., Lubin, J., Weiss, L.M., Bender, C.F., Blake, C.H., Dressing, C.D., Halverson, S., Hearty, F., Howard, A.W., Huber, D., Isaacson, H., Jackman, J.A. ~G., Llama, J., McElwain, M.W., Rajagopal, J., Roy, A., Robertson, P., Schwab, C., Shkolnik, E.L., Wright, J.T., Laughlin, G., 2022. The Aligned Orbit of WASP-148b, the Only Known Hot Jupiter with a nearby Warm Jupiter Companion, from NEID and HIRES. The Astrophysical Journal Letters926, L8.
  • Dalba, P.A., Kane, S.R., Dragomir, D., Villanueva, S., Collins, K.A., Jacobs, T.L., LaCourse, D.M., Gagliano, R., Kristiansen, M.H., Omohundro, M., Schwengeler, H.M., Terentev, I.A., Vanderburg, A., Fulton, B., Isaacson, H., Van Zandt, J., Howard, A.W., Thorngren, D.P., Howell, S.B., Batalha, N.M., Chontos, A., Crossfield, I.J. M., Dressing, C.D., Huber, D., Petigura, E.A., Robertson, P., Roy, A., Weiss, L.M., Behmard, A., Beard, C., Brinkman, C.L., Giacalone, S., Hill, M.L., Lubin, J., Mayo, A.W., Močnik, T., Akana Murphy, J.M., Polanski, A.S., Rice, M., Rosenthal, L.J., Rubenzahl, R.A., Scarsdale, N., Turtelboom, E. V, Tyler, D., Benni, P., Boyce, P., Esposito, T.M., Girardin, E., Laloum, D., Lewin, P., Mann, C.R., Marchis, F., Schwarz, R.P., Srdoc, G., Steuer, J., Sivarani, T., Unni, A., Eisner, N.L., Fetherolf, T., Li, Z., Yao, X., Pepper, J., Ricker, G.R., Vanderspek, R., Latham, D.W., Seager, S., Winn, J.N., Jenkins, J.M., Burke, C.J., Eastman, J.D., Lund, M.B., Rodriguez, D.R., Rowden, P., Ting, E.B., Villaseñor, J.N., 2022. The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope. The Astronomical Journal. 163, 61.
  • Marchis, F., Malvache, A., Marfisi, L., Borot, A., Arbouch, E., 2020. Unistellar eVscopes: Smart, portable, and easy-to-use telescopes for exploration, interactive learning, and citizen astronomy. Acta Astronaut. 166, 23–28.
  • Zellem, R.T., Pearson, K.A., Blaser, E., Fowler, M., Ciardi, D.R., Biferno, A., Massey, B., Marchis, F., Baer, R., Ball, C., Chasin, M., Conley, M., Dixon, S., Fletcher, E., Hernandez, S., Nair, S., Perian, Q., Sienkiewicz, F., Tock, K., Vijayakumar, V., Swain, M.R., Roudier, G.M., Bryden, G., Conti, D.M., Hill, D.H., Hergenrother, C.W., Dussault, M., Kane, S.R., Fitzgerald, M., Boyce, P., Peticolas, L., Gee, W., Cominsky, L., Zimmerman-Brachman, R., Smith, D., Creech-Eakman, M.J., Engelke, J., Iturralde, A., Dragomir, D., Jovanovic, N., Lawton, B., Arbouch, E., Kuchner, M., Malvache, A., 2020. Utilizing Small Telescopes Operated by Citizen Scientists for Transiting Exoplanet Follow-up. Publ. Astron. Soc. Pacific 132, 054401.

Conference Proceedings

 

  • Marchis, F., Esposito, T., Lambert, R., Dalba, P., 2022. New Astronomy with the Unistellar Network, in: IAC 2022 Congress Proceedings, 73rd International Astronautical Congress (IAC), Paris, France.
  • Lambert, R. A., Marchis, F., Asencio, J., Blaclard, G., Sgro, L. A., Giorgini, J. D., Plavchan, P., White, T., Verveen, A., Goto, T., Kuossari, P., Sethu, N., Loose, M. A., Will, S., Sibbernsen, K., Pickering, J. W., Randolph, J., Fukui, K., Huet, P., Guillet, B., Clerget, O., Stahl, S., Yoblonsky, N., Lauvernier, M., Matsumura, T., Yamato, M., Laugier, J.-M., Brodt-Vilain, O., Espudo, A., Kukita, R., Iida, S., Kardel, S., Green, D., Tikkanen, P., Douvas, A., Billiani, M., Knight, G., Ryno, M., Simard, G., Knight, R., Primm, M., Wildhagen, B., Poncet, J., Frachon, T., Shimizu, M., Jackson, A., Parker, B., Redfern, G., Nikiforov, P., Friday, E., Lincoln, K., Sweitzer, J., Mitsuoka, R., Cabral, K., Katterfeld, A., Fairfax, M., 2022. Citizen science astronomy with a network of small telescopes: the launch and deployment of JWST, in: Marshall, H.K., Spyromilio, J., Usuda, T. (Eds.), Ground-Based and Airborne Telescopes IX, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. p. 121822Z.

  • Marchis, F., Esposito, T., Peluso, D., Blaclard, G., Asencio, J., Megowan-Romanowicz, C., Pennypacker, C., Carter, B., 2021. Outreach and scientific Results With The Largest Network of Backyard Astronomers — IAF Digital Library, in: IAC 2021 Congress Proceedings, 72nd International Astronautical Congress (IAC), Dubai, United Arab Emirates.
  • Barbosa, D., Coelho, B., Bergano, M., Magalhães, C., Mendonça, D., Silva, D., Correia, A., Pandeirada, J., Ribeiro, V., Esposito, T., Marchis, F., 2021. Cyber-Cosmos: a new Citizen science concept in a Dark Sky Destination — IAF Digital Library, in: IAC 2021 Congress Proceedings, 72nd International Astronautical Congress (IAC), Dubai, United Arab Emirates.

Conference Abstracts

  • Graykowski A., Lambert R. A., Marchis F., Cazeneuve D., Dalba P. A., et al. 2023. Citizen Science Observations of the Ejecta from Dimorphos after the DART Impact. in: Asteroids, Comets, Meteors Conference Abstracts. #2297
  • Graykowski, A., Lambert, R.A., Marchis, F., Esposito, T. M., Sgro, L. A., Weaver, I., Peluso, D. O’C., Dalba, P. A. 2023. Monitoring Variable Cometary Activity with Citizen Science Using the Unistellar Network. in: AAVSO 112 Annual Meeting Abstracts
  • Graykowski, A. and Marchis, F. 2023. Monitoring Cometary Activity and Characterizing the Outbursts of 29P/Schwassmann–Wachmann and 12P/Pons-Brooks using Citizen Science Observations. in: AGU Fall Meeting Abstracts. pp. P44B-07
  • Hanuš, J et al., 2023 Stellar Occultation by Asteroids: the contribution of Unistellar’s network of citizen astromnomers, 55th Annual Meeting of the Division for Planetary Sciences, 312.04, Vol. 55,8
  • Bruno Guillet, Tom Esposito, Arin Avsar, Franck Marchis, Daniel Peluso, and 130 citizen astronomers, 2022. Détections d’exoplanètes par des astronomes amateurs du réseau Unistellar, Posters aux journées 2022 de la SF2A, Besançon (France) Juin 2022
  • Bruno Guillet, Franck Marchis, Joé Asencio, Ryan Lambert, Paul Dalba, Guillaume Blaclard, and several citizen astronomers, 2022. Détections d’astéroïdes et d’engins spatiaux par des astronomes amateurs du réseau Unistellar, Posters aux journées 2022 de la SF2A, Besançon (France) Juin 2022
  • Esposito, T., Avsar, A., Marchis, F., Dalba, P., Peluso, D., 2022. Hot and Cold Jupiters: Exoplanet Transit Results from the Unistellar Citizen Scientist Network, in: American Astronomical Society Meeting Abstracts, American Astronomical Society Meeting Abstracts. p. 339.07.

  • Hanus, J., Marchis, F., Asencio, J., Durech, J., 2021. Lightcurve observations of near-Earth asteroids with the Unistellar’s network of citizen astronomers, in: AGU Fall Meeting Abstracts. pp. SY55C-0361.

  • Marchis, F., Esposito, T., Asencio, J., Klavans, V., Blaclard, G., Peluso, D.O., Megowan-Romanowicz, C., Pennypacker, C., 2021. Citizen Science and Scientific Results from the Worlds Largest Network of Backyard Astronomers, in: AGU Fall Meeting Abstracts. pp. SY55A-04.
  • Hanus, J., Durech, J., Marchis, F., Asencio, J., Blaclard, G., 2021. Physical Properties of Near-Earth Asteroids, in: AGU Fall Meeting Abstracts. pp. P33A-02.

  • Cazeneuve, D., Marchis, F., Blaclard, G., Asencio, J., Martin, V., 2021. Detection of Occultation Events by Machine Learning for the Unistellar Network, in: AGU Fall Meeting Abstracts. pp. P11B-12.

  • Marchis, F., Asencio, J., Peluso, D., Durech, J., Vereš, P., Blaclard, G., Demuys, I., Nachury, L., 2021. The Contribution of the Unistellar Network for Planetary Defense: Empowering Crowd-sourcing Astronomy, in: 7th IAA Planetary Defense Conference. p. 271.

  • Dunham, D., Dunham, J., Buie, M., Preston, S., Herald, D., Farnocchia, D., Giorgini, J., Arai, T., Sato, I., Nolthenius, R., Irwin, J., Degenhardt, S., Marshall, S., Moore, J., Whitehurst, S., Venable, R., Skrutskie, M., Marchis, F., Ye, Q., Tanga, P., Aissa, D.B., Grigahcene, Z., 2021. Accurate NEO Orbits from Occultation Observations, in: 7th IAA Planetary Defense Conference. p. 37.

  • Esposito, T. M., Avsar, A., Peluso, D., Marchis, F., Santana, P., Klavans, V., Nachury, L., 2021. TESS Planet Candidate Follow-up by Citizen Scientists in the Global Unistellar eVscope Network, in: Posters from the TESS Science Conference II (TSC2), held virtually, id.155. .

  • Marchis, F., Peluso, D., Esposito, T., Megowan-Romanowicz, C., Pennypacker, C., Unistellar Science Team, 2021. A Large Citizen Science Astronomy Network for All of Us, in: American Astronomical Society Meeting Abstracts, American Astronomical Society Meeting Abstracts. p. 412.06.
  • Esposito, T. M., Marchis, F., Peluso, D., Avsar, A., Zellem, R. T., 2021. Transiting Exoplanet Followup by Citizen Scientists with the Global Unistellar eVscope Network, in: American Astronomical Society Meeting Abstracts, American Astronomical Society Meeting Abstracts. p. 239.03.
  • Asencio, J., Marchis, F., Esposito, T., Veres, P., 2020. Planetary Defense With a Network of Compact, Smart and Low-Cost Digital Telescopes, in: AGU Fall Meeting Abstracts. pp. NH037-0008.
  • Marchis, F., Esposito, T., Asencio, J., Demuys, I., Peluso, D., Veres, P., Zellem, R., Nachury, L., 2020. Enabling and Empowering Citizen Science in Astronomy With a Network of Small Digital & Smart Telescopes, in: AGU Fall Meeting Abstracts. pp. ED025-06.

  • Marchis, F., Esposito, T., Asencio, J., Demuys, I., Peluso, D., Veres, P., Zellem, R., Hanus, J., Nachury, L., 2020. First Results With a Network of Small Digital & Smart Telescopes: Citizen Science For Astronomy, in: AAS/Division for Planetary Sciences Meeting Abstracts, AAS/Division for Planetary Sciences Meeting Abstracts. p. 413.02.

  • Marchis, F., Esposito, T., Malvache, A., Peluso, D., Vereš, P., Hanuš, J., 2020. Unistellar: The largest citizen science astronomy network for all of us — IAF Digital Library, in: IAC 2020 Congress Proceedings, 71st International Astronautical Congress (IAC) — IAC CyberSpace Edition , 12–14 October 2020.

  • Marchis, F., Arbouch, E., Peluso, D., Harman, P. K., Malvache, A., Bertin, E., Zellem, R., Veres, P., 2019. Citizen Science Astronomy with the Unistellar Network: From Planetary Defense to Exoplanet Transits, in: AGU Fall Meeting Abstracts. pp. ED14A-03.

  • Marchis, F., Arbouch, E., Bertin, E., Malvache, A., Vereš, P., Zellem, R.T., 2019. Citizen Science Astronomy with the Unistellar Network: From Planetary Defense to Exoplanet Transits, in: EPSC-DPS Joint Meeting 2019. p. EPSC-DPS2019-898.

Further readings

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When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope /en-eu/blog/annular-solar-eclipse-2023/ Fri, 06 Oct 2023 14:48:22 +0000 /blog/annular-solar-eclipse-2023/ An annular solar eclipse is visible from the Americas on October 14. Learn how to witness the Ring of Fire with your Unistellar Telescope!

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You can observe a solar eclipse not once, but twice within the next year in North America. This double-whammy kicks off with an annular solar eclipse on October 14, 2023, and finishes with a total solar eclipse on April 8, 2024. Solar eclipses occur thanks to a fortunate alignment of the Moon and Sun, and can be observed quite easily (with the proper protection!). If you have a Unistellar telescope with a , you’ll be able to get an up-close look at the first of these celestial alignments very soon!

Even if you’re not in the eclipse’s wake on October 14 (or you have bad weather, an astronomer’s worst nightmare!), you can still view the annular eclipse virtually. Join the SETI Institute and Unistellar on or for a special SETI Live event, where we will livestream the eclipse from within the path and talk with solar experts!

Credits: NASA. The umbra marks the deepest part of the moons shadow, where a total or annular eclipse occurs in the path of totality/annularity. The penumbra is the outer part of the shadow, and causes a partial eclipse where it falls.

What is a Solar Eclipse?

A solar eclipse occurs when the Moon passes in front of the Sun, as seen from Earth. This blocks the Sun’s light, casting the Earth’s surface into darkness for several minutes. Birds roost and insects may begin to sing, thinking it’s night, and the temperature will drop noticeably. Globally, eclipses usually occur several times per year, but they can only be seen in their full glory from a specific area, called the path of totality (or annularity). An area outside the path may see a partial eclipse depending on its proximity to the path.

Aside from partial eclipses, there are two main types of solar eclipses. A total solar eclipse, like the one that will be visible from North America next year, occurs when the Moon fully blocks the Sun’s disk. During total solar eclipses you can see the Sun’s corona, or hot outer atmosphere, which is normally not visible.

However, the upcoming solar eclipse of October 14, 2023 will be an annular solar eclipse, meaning the Sun will not be fully blocked. It’s still an amazing sight to behold, however, and well worth watching! An annular eclipse occurs when the Moon is directly in front of the Sun but doesn’t appear large enough to fully cover it, instead creating what’s called the “Ring of Fire,” as the Sun’s outer edge remains visible. The portion of the eclipse where the Ring of Fire is visible is called “annularity.” Leading up to annularity, onlookers will be able to view a partial eclipse as the Moon gets in position to block the Sun. When the annularity is finished, viewers will again witness a partial eclipse as the Moon moves out of the way.

 

The stages of an annular eclipse. A partial eclipse occurs before and after the moon is located directly in front of the Sun’s disk. Credit:

When is the Next Solar Eclipse? From Where Can You See the Next Solar Eclipse?

The path of the will begin on the Oregon coast and move southeast, crossing Nevada, Utah, New Mexico, and Texas in the US before moving over the Gulf of Mexico. This 2023 solar eclipse will then cross Mexico’s Yucatan Peninsula and parts of Central America before sweeping across Columbia and northern Brazil.

You’ll be able to see a partial annular solar eclipse from anywhere in the United States, meaning the Sun will be at least partly covered by the Moon. The Sun will appear to be more fully covered the closer you get to the eclipse’s path, and if you’re in the path, you will see the moon fully in front of the Sun. Plus, the closer you get to the center of the path, the longer you will be able to see the Ring of Fire! At the very center of the path, annularity will last about 4.5 minutes, but it will last for a shorter time toward the edges of the path.

The partial eclipse will start around 8am PDT from the Oregon coast, but the time to start observing will change depending on location. So to see whether you’ll be able to view the annular eclipse, and when, check out or this resource.

It’s important to remember not to look directly at the Sun without proper eye protection at any point during an annular eclipse! Because the Sun is not fully covered, it can still harm your eyesight. You can use eclipse glasses or a for your telescope to safely view the Sun.

The path of the October 14, 2023 annular eclipse. The yellow circle denotes the Sun’s shadow as it begins to cross the continent. Yellow lines marked by a percentage denote how much of a partial eclipse will be visible from the area. Credit: .

How to Watch a Solar Eclipse With a Unistellar Telescope

A Unistellar Telescope outfitted with a Smart Solar Filter is perfect for viewing the Sun during an eclipse. You can watch the Moon slowly slide over the Sun, observe the Ring of Fire at annularity, and spy on the solar corona during a total solar eclipse.

The first step in observing the Sun with your Unistellar telescope is to make sure your App is updated to version 2.5. Then, you can prepare for the eclipse by setting up your telescope (keep the dust cap on!) and taking the following steps at least 15 minutes before the start of the eclipse from your location. If you need more instructions, you can find a detailed account of the Solar Experience setup at our

  1. Select the Sun in the App Catalog – Once connected to your telescope’s WiFi, open the Unistellar App and select the Sun. Click GoTo and you will be prompted with a short tutorial that contains the following steps. There is no need for an Orientation to select the Sun from the App Catalog.
  2. Check your solar filter – Make sure your Smart Solar Filter is free from scratches or holes.
  3. Place the solar filter – Remove the dust cap and promptly place the Smart Solar Filter on the top of the telescope.
  4. Manually position the telescope – Unscrew the tripod screws and manually position your telescope mount in the direction of the Sun; the structure with the motor must be to your right once you are facing the Sun. Once the telescope is facing the Sun with the structure at your right, do not forget to tighten the tripod screws.
  5. Start the solar observation – Click on « GoTo » again to automatically align the telescope with the Sun and track it.

 

Unistellar Smart Solar Filter

You will get a confirmation message when your telescope is centered on the Sun. Now you are ready to observe the eclipse! You may want to record your screen on your smart device to see the eclipse in action.

Remember, just as it is never safe to look directly at the Sun without the proper eye protection, it is never safe for your telescope to be pointed at the Sun without the Smart Solar Filter. Exposure to the Sun without our Smart Solar Filter will cause damage to the sensor, just like it would damage your eyes.

Please share your wonderful eclipse photos with us on social media. Don’t forget to tag @Unistellar! Happy sun-gazing!

Further readings

The post When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope appeared first on .

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Halloween Observing Guide: Spooky Deep-Sky Objects /en-eu/blog/observe-october-2023/ Sat, 30 Sep 2023 03:03:36 +0000 /blog/observe-october-2023/ These Halloween deep-sky objects will add some light to those dark, spooky nights. Treats, tricks, and telescopes await!

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Step outside on a crisp October evening, and you’ll find the heavens adorned with celestial wonders that seem tailor-made for the Halloween season. From eerie-shaped clusters to cosmic apparitions, this month’s night-sky spectacles will send shivers down your spine.

Follow our Halloween observing guide to enjoy some of these boo-tiful deep sky objects as you prepare for tricks, treats, and Unistellar telescopes!

 

All-Level Targets

These bright objects are easy for anyone to observe, and some are visible from both hemispheres!

Wizard Nebula (NGC 7380)

If you’ve ever noticed the “man on the moon,” you’ll be glad to meet the wizard in the clouds! Clouds of cosmic gas and dust, that is. With its wispy tendrils, the Wizard Nebula cradles a young star cluster that has been forming from the material that makes up this star-forging region. These new stars have carved out a shape in the surrounding nebula that appears to be a wicked wizard’s face. Can you see it? Try from the Northern Hemisphere!

The Wizard Nebula imaged and processed by John Bradley.

Tarantula Nebula

The Tarantula Nebula, residing in the Large Magellanic Cloud galaxy, might give you astronomical arachnophobia. This vast cloud of gas and dust is illuminated by the fierce light of some of the hottest and most massive new stars known to us humans. The stars’ powerful radiation clears out all but the most dense clouds and casts an eerie, spider-like silhouette against the cosmic canvas. Spot this creepy creature from the Southern Hemisphere.

Tarantula Nebula

The Tarantula Nebula, imaged by the Unistellar team.

Ghost Bush Cluster (NGC 6939)

The Ghost Bush Cluster, NGC 6939, is an open star cluster located in the constellation Cepheus and is best seen from the Northern Hemisphere. It’s quite an old open cluster at over 1 billion years of age, but it and its nearby neighbor – the Fireworks Galaxy – still make a striking pair.

Why is it sometimes called the Ghost Bush Cluster? Well, Halloween is for mysteries after all. Likely it was named for the stunning (but slightly spooky) plant!

Eagle

The Ghost Bush Cluster imaged by Unistellar observer Michel Dubeau.

Owl Cluster (aka E.T. Cluster)

The E.T. cluster, better known as the Owl Cluster, is an open cluster in the constellation Cassiopeia. Its brightest stars might remind you of the eyes of an owl, or if you’ve been hanging around SETI Institute scientists, those of a certain extraterrestrial from the movie E.T. Best viewed from the Northern hemisphere. See what you think! Is it avian or other-worldly?

The Owl/E.T. Cluster imaged and processed by Richard Bright.

Mirach’s Ghost

Mirach’s Ghost is an intriguing celestial duo located in the constellation Andromeda. This ethereal pairing consists of Mirach, the brightest star in Andromeda, and a faint, ghostly dwarf galaxy named NGC 404. Take a dark October night to gaze upon Mirach and catch a glimpse of its spectral companion! To spot it, simply use the Unistellar App to GoTo Mirach – you will see NGC 404 lurking next to the bright star it in the field of view.

Mirach imaged by David Rowe. You can see the fuzzy-looking Mirach’s Ghost, NGC 404, above the star and to the left!

There’s plenty of other great targets to see this month, creepy or not! From the Northern Hemisphere, check out the White Rose Cluster, often called Caroline’s Rose or the Ghost Cluster. In the Southern Hemisphere you can see the Bat Nebula in the later half of the night!

Challenge Targets

For more challenging targets, find these next few frightening objects! These are dimmer or more diffuse celestial sights that you may need to observe via Enhanced Vision for longer than the All-level targets if you want to experience their full, eerie effects.

Superman Galaxy (NGC 7479)

Not all things Halloween have to be scary! NGC 7479, affectionately dubbed the Superman Galaxy due to its distinctive ‘S’ shape, is a barred spiral galaxy located in the constellation Pegasus. This cosmic superhero showcases its stunning, nearly symmetrical spiral arms, making it a heroic sight in the night sky. Also known as the Propeller Galaxy, it’s perfect for thrill-seeking stargazers in both hemispheres.

The Superman Galaxy imaged and processed by Unistellar observer John Short.

Skull Nebula (NGC 246)

This ghoulish nebula from the Cetus constellation is a Southern Hemisphere favorite. It’s a planetary nebula, meaning it was born from a dying sun-like star – but that’s not why it’s called the Skull Nebula! Although somewhat faint, a bit of time on target will reveal what some see as the shape of a spooky skull or a ghostly “Pac-Man.”

The Skull Nebula, imaged by Unistellar observer David Hein.

The Bubble Nebula (NGC 7635)

The Bubble Nebula, also known as NGC 7635, is an emission nebula found in the constellation Cassiopeia. Although not traditionally terrifying, its ethereal, bubble-like appearance, formed by the stellar winds of a massive star at its center, invokes mystical ambiance fitting for October nights in the Northern Hemisphere. Perhaps they are bubbles from a cosmic cauldron!

A composite image of the Bubble Nebula by the Unistellar Team.

 

We encourage you to share your Halloween-time observations and join the conversation through our Facebook, Instagram and Twitter pages. Don’t forget to tag @Unistellar!

If you’d like to send us your observations by email, send them tocommunity@unistellaroptics.com.

Clear skies and stay spooky!🔭

Further readings

The post When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope appeared first on .

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How Big Is the Solar System? /en-eu/blog/how-big-is-the-solar-system/ Wed, 27 Sep 2023 23:55:15 +0000 /blog/how-big-is-the-solar-system/ If the Sun were the size of a basketball, do you know how big the Earth would be? Find out how big the Solar System really is!

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Our solar system is filled with planets, asteroids, comets, dwarf planets and trillions of other small objects all orbiting a mid-sized star that we call the Sun. The solar system has eight planets including Earth, a main asteroid belt and regions farther out beyond the planets where countless small objects orbit.

While astronomers have studied much of what makes up our solar system, a lot of space nearby remains unexplored, including many more objects surely to be found in our neighborhood. Part of the reason for this mystery is that our solar system is really, really big – at least in human terms! For example, the Earth is 150 million kilometers (93 million miles) away from the Sun — a distance astronomers call an astronomical unit (AU) — which would take an airliner flying at a typical speed around 20 years to cover. Neptune, the farthest planet, is around five billion km (3 billion mi) from the Sun.

The solar system is so large that when thinking about how big the solar system is, we need to shrink the Sun and planets down far tinier than they really are to comprehend it — and even then it’s still hard to wrap your mind around! From the edge of the Solar System, Earth would just be a pale, blue dot.

An updated version of the famous “Pale Blue Dot” image. This image was taken by the Voyager 1 spacecraft while it was out past the orbit of Neptune. Through rays of scattered light you can see the Earth as just a pale, blue dot.

What is in our Solar System?

The solar system has eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. Pluto, formerly known as the ninth planet, was reclassified as a dwarf planet in 2006. Our Solar System also has a large asteroid belt that’s filled with millions of asteroids ranging in size from a pebble to hundreds of kilometers across. How big is the asteroid belt? It spans about 225 million km (140 million mi) and is located between Mars and Jupiter.

Beyond Neptune is the Kuiper Belt, which extends from 30 to 55 AU (8.2 billion km or 5.1 billion mi). The Kuiper Belt is filled with small, rocky and icy objects, and it’s where many short-period comets likely come from. Pluto can be found in the Kuiper Belt, along with three other dwarf planets, and potentially many more. Astronomers are actively searching the Kuiper Belt for new objects.

Outside of the Kuiper Belt is a vast region called the Oort Cloud, where trillions of small, icy objects orbit, loosely held by the Sun’s gravity. Whereas the Kuiper Belt orbits in the same plane as the planets, the Oort cloud is more like a shell encompassing our Solar System. Minor planets, dwarf planets, comets and other objects also inhabit the Oort Cloud, though astronomers don’t know all that much about what lives so far from the Sun.

Jupiter

Jupiter, our largest planet, as imaged through a Unistellar eVscope. The great red spot is visible towards the bottom. You can even see a few of its moons in the image!

With a Unistellar Telescope, you can see all seven other planets, and even many comets and asteroids in our Solar System. Observe Saturn’s rings, Jupiter’s great storms and spy on distant Uranus and Neptune, all from your backyard. Smaller objects like asteroids become visible when they occult, or pass in front of, distant stars. Unistellar hosts multiple observing campaigns every year targeting asteroids and other distant objects to help scientists keep an eye on nearby ones and learn more about distant ones.

Where is the edge of the Solar System?

The Oort Cloud starts somewhere between 1,000 and 5,000 AU from the Sun, and extends to around 100,000 AU, or about 15 trillion km (9.3 trillion miles), away, although some estimates place it closer to the Sun and some almost twice as far. The far edge of the Oort Cloud is considered the edge of our Solar System, making our cosmic neighborhood quite big indeed. So, to find how big the solar system is across, we could double that distance, giving us a rough estimate for a diameter of 200,000 AU, or 30 trillion km (18.6 trillion miles). That’s over 3 light years across!

A Solar System size comparison

Typical diagrams of the solar system showing all of the planets don’t really do our cosmic neighborhood justice. The solar system is so big that the planets would be tiny dots, spread so far from each other that it would be impossible to put them all next to each other. To understand how big the solar system is, it’s helpful to compare the Sun and planets to everyday objects.

For example, let’s shrink the Sun to the size of a basketball. In this scenario Mercury, the first planet, would be less than a millimeter across, and located about one meter (3 ft) from the Sun. Venus, the next planet, would be just under two millimeters in size, and about 18 meters (60 ft) away. Our Earth would be 25 meters (80 ft) away, and a bit bigger than Venus, about the size of a small bead. Next up is Mars, at 38 meters (125 ft) away and about one millimeter across.

The approximate sizes of the planets in relation to each. The Sun is so large that, if it were shown, the terrestrial planets would be just small dots! In order from left to right, or closest to farthest from the Sun): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto (for reference!) Credit: NASA/Lunar and Planetary Institute

Jupiter, the largest planet, would be just about the size of a quarter or euro, at 2.4 centimeters, and 130 meters (425 ft) away from the basketball Sun (more than the length of a football field). Saturn would be 1.9 cm across (or roughly the size of a nickel), and 240 meters (790 ft) away, while Uranus would be 0.8 cm across and 480 m (1,575 ft) away. Neptune, the farthest planet, would be 0.9 cm across, and an incredible 750 m (2,460 ft, around half a mile) away. For our imperial system users, both Uranus and Neptune would be less than a half inch across in this basketball “solar system”.

The edge of the Oort Cloud – the edge of the Solar System – would sit around 2,500 km (1,500 mi) distant from the basketball in this scenario . That’ about the length of the east coast of the U.S! So if our basket-ball sized Sun was in Miami, Florida, the Solar System’s outer reaches would extend all the way to Portland, Maine.

How you can explore the Solar System

Though the Solar System is quite large, you can explore its vast reaches from the comfort of your backyard. Consumer telescopes are powerful enough to bring the planets into crisp detail, explore craters on the Moon and see comets and other objects passing by Earth. With a Unistellar Telescope, you can observe even from bright cities thanks to our Deep Dark Technology, which reduces the effects of light pollution. Plus, you can now even observe the Sun with our Solar Experience! So you can voyage through every aspect of our star system from here on Earth.

Skygazing isn’t just for pleasure, either. Scientists exploring our Solar System need the help of Citizen Astronomers, who make observations of planets, asteroids and even spacecraft to better understand them. Unistellar Network members keep an eye on Near-Earth Asteroids to aid Planetary Defense, observe passing comets to refine their orbits and scan the outer reaches of the Kuiper Belt and Oort Cloud for new minor planets. Learn more about how you can explore our vast, wonderful Solar System!

Further readings

The post When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope appeared first on .

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See OSIRIS-REx, NASA’s First Asteroid Sample Return Mission, as it Drops off Pieces of Asteroid Bennu /en-eu/blog/observe-osiris-rex/ Fri, 15 Sep 2023 17:00:16 +0000 /blog/see-osiris-rex-nasas-first-asteroid-sample-return-mission-as-it-drops-off-pieces-of-asteroid-bennu/ NASA's first asteroid return sample mission, OSIRIS-REx, is headed back towards Earth with precious cargo. Join us in observing it Sept. 24!

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Update: The Unistellar Network successfully observed OSIRIS-REx! See below for some of their observations. Left – Darren Rivett in Australia observed OSIRIS-REx just minutes before it released the capsule of asteroid samples. Right – Keiichi Fukui in Japan observed the spacecraft as it sped away from Earth after the release.

Journeying millions of miles from Earth, navigating the vast, cold expanse of space, and finally touching an ancient celestial body—this isn’t the plot of a sci-fi novel, but the real-life saga of NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security-Regolith r). This mission, launched in September 2016, wasn’t just about reaching the near-Earth asteroid Bennu; it was about extracting a piece of our Solar System’s history.

The highlight of the OSIRIS-REx mission occurred in October 2020, when the spacecraft executed a “Touch-And-Go” (TAG) maneuver with Bennu. During this intricate operation, the spacecraft briefly touched the asteroid’s surface to collect a sample. The success of this operation was monumental, marking the first time NASA collected a sample from an asteroid. And on September 24, just over 7 years from its OSIRIS-REx’s launch, that piece of Bennu is coming back home.

Why Potentially-Hazardous Asteroid Bennu?

Bennu was not chosen by accident for the OSIRIS-REx mission; its selection was the result of careful consideration and scientific motivations. As a carbon-rich asteroid, Bennu may carry clues to the origins of life, since carbonaceous material is believed to be a key ingredient in the primordial soup that led to life on Earth.

 

PHA Bennu imaged by Osiris-REx right before arrival. Credit: NASA/Goddard/University of Arizona

Since it has been preserved in the vacuum of space for billions of years after its birth in the Asteroid Belt, Bennu acts as a time capsule carrying the history of the Solar System. Therefore, studying its composition can provide scientists with a peek at the materials present when life formed on Earth. This, in turn, can help us understand the processes that might have led to the formation of organic molecules, and possibly even life, on our planet.

Bennu is a nearby and also sizable asteroid at about 500m in diameter, which makes it not only a near-Earth asteroid but a potentially hazardous one! Furthermore, Bennu’s orbit carries a slight risk of impacting Earth in the late 22nd century (don’t fret – there’s only a 1 in 2,700 chance of impact between the years 2175 and 2199!) so studying it up close also provides valuable planetary defense data about its prior interactions and future trajectory. Between its size, suspected composition, and placement, Bennu is the perfect target for OSIRIS-REx.

Asteroid Bennu’s size compared to famous landmarks. Credit: University of Arizona

The OSIRIS-REx Mission

OSIRIS-REx took over 2 years to reach its target over a million miles away, but the result was well worth the wait. Once the craft reached Bennu in December 2018, it spent its time mapping out the asteroid so that the mission team could pick the best spot to extract a sample. The team eventually settled on site in a recently formed crater that would allow them to safely obtain the most pristine sample possible, one that holds the history of Bennu. On October 20, 2020, the OSIRIS-REx mission made NASA history when it successfully gathered enough material from Bennu during its TAG maneuver.

An artist’s conception of OSIRIS-REx making contact with Bennu during the “TAG” Manuever. – and it’s as cool as it sounds! Studies show that, because Bennu is a rubble-pile asteroid, OSIRIS-REx could have fallen into it after the maneuver if it had not thrusted in the opposite direction. Credit: NASA/University of Arizona

After completing some more scientific observations, OSIRIS-REx made its way back home in April 2021. Now for the exciting part – it’s due to reach Earth on September 24, 2023, where it will release its precious cargo at 10:42 UTC! But it won’t be slowing down in order to make the historic dropoff – instead, as it flies 63,000 miles (102,000 km) over the Earth’s surface, it will release the capsule of Bennu samples. After 4 hours of hurtling through space, the sample capsule will finally enter Earth’s atmosphere at 14:42 UTC. From high in the sky it will drift to the ground helped by a series of parachutes, landing approximately 13 minutes later at the US Department of Defense’s Utah Test and Training Range where it will be collected by scientists anxiously awaiting its arrival.

Only 20 minutes after the sample capsule is jettisoned into space, the OSIRIS-REx spacecraft will divert away from Earth as it heads towards its next target, near-Earth asteroid Apophis, ushering in the new age of OSIRIS-APEX (OSIRIS-APophis EXplorer). Although Apophis is not as large as asteroid Bennu, it is scheduled to come within 20,000 miles (32,000 km) of Earth in 2029. OSIRIS-REx turned OSIRIS-APEX will take advantage of the opportunity and orbit Apophis after the approach, studying its surface and looking for any disturbances caused by its Earthly flyby.

How Can You Observe OSIRIS-REx?

Various locations on Earth will be able to catch OSIRIS-REx for a short time as it gets in position to drop the capsule at 10:42 UTC (we encourage you to observe at the moment of release! If you want to try to observe the capsule, scroll to the bottom of this section). You can continue to observe OSIRIS-REx for several hours after the release as it diverts away from Earth and towards Apophis. In summary, the visibility window lasts from about 09:00 to 14:00 UTC, with best visibility occurring between 10:00 and 12:00 UTC.

At approximately 09:00 UTC, OSIRIS–REx will be getting closer to Earth and therefore bright enough to observe. Check the map below to see if it will be visible to you at this time – if you are in the blue area, you should be able to see it!

A visibility map of OSIRIS-REx at 09:00 UTC on September 24. The pink areas mark daylight, but anyone located in the blue region should be able to see the spacecraft at least 10 degrees above the horizon.

Several hours later at approximately 13:00 UTC, OSIRIS-REx will have set for the Americas but will be visible from Japan and the West coast of Australia. By the time it is visible to these locations, it will be moving very fast as it heads towards its next target, so the spacecraft may leave the field of view after only a few minutes – catch it while you can!

A visibility map of OSIRIS-REx at 13:00 UTC on September 24. By this point, OSIRIS-REx will be moving very quickly as it diverts its path towards Apophis.

To observe OSIRIS-REx with your Unistellar Telescope, follow the instructions on our Planetary Defense Tutorial page and scroll down to option B: The Planetary Defense target is not in the Unistellar App’s database. This will instruct you on how to use our Moving Target Ephemeris page to plan your observation of OSIRIS-REx using the Planetary Defense science mode. This page will provide Deep Links that open the Unistellar app and contain all the observing parameters you need to make a 10-minute long science observation. Notice that the Deep Links will only be available when the target is visible to you – if the target is not visible, a crossed-out eye icon will appear. You can therefore use the Ephemeris page and this feature to determine exactly when OSIRIS-REx will be observable from your location.

Because OSIRIS-REx will be moving so fast, we suggest that you plan your observation ahead of time. For instance, if you use the Moving Target Ephemeris page to generate a Deep Link for September 24th at 09:00 UTC, make sure that you are outside and have already clicked GoTo so that your telescope is aimed at the correct location by 09:00! We also encourage you to take Enhanced Vision images, as you may see OSIRIS-REx streak across the field of view.

If you would like to try to observe the OSIRIS-REx capsule, which is also on the Moving Target Ephemerids page, check out the youtube video below. This is a special observing case which will require some special steps, so follow the instructions outlined in the video and check out our Citizen Science Slack Workspace to communicate with other observers seeking to view the event. If you have any questions, please reach out to us at citizenscience@unistellaroptics.com.

Further readings

The post When Is the Next Solar Eclipse, and How to Observe It With a Unistellar Telescope appeared first on .

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Fall Into Cygnus and More With September Deep-Sky Objects /en-eu/blog/observe-september-2023/ Wed, 30 Aug 2023 15:50:03 +0000 /blog/observe-september-2023/ Unistellar’s September targets include a bevy of star clusters and nebulae of all sorts. Celebrate stars in all stages of life this month!

The post Fall Into Cygnus and More With September Deep-Sky Objects appeared first on .

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A new month brings a new crop of celestial wonders for astronomers everywhere to view. This September brings a flurry of nebulae and star clusters with it, meaning you’ll be able to get your fill of stars in all stages of life this month! We’ve got some of each for you to find with your Unistellar Telescope, including one cluster with a curiously missing centerpiece.

Many of these September sights lie in the constellation Cygnus the Swan, which hosts a rich tapestry of deep sky objects due to its location on the galactic plane. This stellar pattern is one of the Northern hemispheres’ high-in-the-sky Autumn gems, but is still visible for some Southern hemisphere observers (it will be quite low on the horizon for those at very Southern latitudes). So let’s dive into the Swan and its neighbors to visit the fascinating targets that this month has to offer.

All-Level Targets

These bright objects are easy for anyone to observe, and many are visible from both hemispheres!

Albireo

Turn your telescope to the head of Cygnus the Swan, the gleaming double star Albireo. The two stars that make up this pair appear with different colors through a telescope, as one is much hotter than the Sun and one much cooler.

Because this star is so bright, you can choose whether or not to use Enhanced Vision. If you want to see the clear separation between the stars, you may instead use the “Edit” button at the bottom of your live view screen to reduce the Gain and Exposure time of the image. This will allow you to better tell the stars apart.

Albireo captured by David Rowe with Enhanced Vision.

M39

Find this open cluster in the constellation of Cygnus. It’s near the bright star Deneb, the tail of the Swan, which can be helpful for locating the cluster. M39 is part of both the Northern Cross and the Southern Triangle – two of the most well-known asterisms in each hemisphere!

Eagle

M39 imaged by Unistellar observer Michel Dubeau.

Cocoon Nebula

Sitting at the edge of Cygnus the Swan, the folds of the Cocoon Nebula shelter a region of young and still-forming stars that burns brightly. Peer closely into this forge of star creation and imagine the fiery conditions within.

The Cocoon Nebula imaged and processed by David Rowe.

Angelfish Cluster (M71)

Visible from both hemispheres, the Angelfish Cluster in Sagitta straddles the line between an open cluster and a globular cluster. The difference between these two types of cluster is namely their age and concentration of stars – open clusters are not as dense and contain younger stars, while globular clusters contain older, densely packed stars. Scientists eventually settled on designating the Angelfish as a young, loosely concentrated globular cluster. See what you think!

The Angelfish Cluster, imaged by Unistellar observer Emmanuel Marchal.

Summer Beehive (IC 4665)

Not to be confused with the well-loved Beehive Cluster of the constellation Cancer, the Summer Beehive Cluster lies in Ophiucus. This lovely open cluster is often called Poseidon’s Trident Cluster – can you spot this familar shape? Catch it as soon as dark falls from both hemispheres.

The Sumer Beehive imaged and processed by John Bradley.

There’s plenty of other great targets to see this month. For example, both the Fireworks Galaxy and the Veil Nebula are primely placed in Cygnus, and other dim nebulae like the Little Ring Nebula (NGC 6894) may pose a fun challenge. Check you Unistellar app catalog to see what’s up in the sky!

Challenge Targets

For more challenging targets, find these next three objects! These are dimmer or more diffuse celestial sights that you may need to observe via Enhanced Vision for longer than the ones in the previous section if you want to see all them in all their glory!

The Hole in the Cluster (NGC 6811)

Also known as NGC 6811, this open cluster in Cygnus contains a mysterious absence of stars near its very center. See if you can spot this dim “smoke ring of stars,” and ponder the inky blackness of space!

The Hole in The Cluster imaged by the Unistellar team.

Crescent Nebula (NGC 6888)

At the heart of this emission nebula, which also lies in Cygnus, you’ll find a rare Wolf-Rayet star – a massive star that’s been living fast and is on its way to dying hard as it burns heavier elements for fuel after it used up all of its hydrogen. This star emits strong stellar winds that whip the clouds of gas and dust in the Crescent Nebula into complex shapes. After several minutes of Enhanced Vision, you should see its half-circle structure begin to appear!

The Crescent Nebula imaged and processed by Matthieu Carbon.

Iris Nebula (NGC 7023)

This reflection nebula glows from within, lit from a star hidden by its gaseous shrouds. Filaments of red indicate an unknown molecule in the Iris Nebula’s clouds, which stretch about six light-years across. This nebula is in the constellation Cepheus, so it’s best seen from the Northern Hemisphere.

The Iris Nebula imaged and processed by Richard Bright.

NGC 6951

For an additional challenge, look for this barred spiral galaxy in the constellation of Cepheus. Persistence will reward you with views of a less-often-spotted galaxy with a distinct shape that’s home to active star formation. Only visible from the Northern Hemisphere.

NGC 6951 imaged by Jacques Bérard & Nicole Ruel back in 2021, when a supernova was spotted to have erupted in this galaxy!

 

We encourage you to share your observations and join the conversation through our Facebook, Instagram and Twitter pages. Don’t forget to tag @Unistellar!

If you’d like to send us your observations by email, send them tocommunity@unistellaroptics.com.

Clear skies!🔭

Further readings

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