January’s Night Sky Notes: The Red Planet

January’s Night Sky Notes: The Red Planet

3 min read

January’s Night Sky Notes: The Red Planet

by Kat Troche of the Astronomical Society of the Pacific

Have you looked up at the night sky this season and noticed a bright object sporting a reddish hue to the left of Orion? This is none other than the planet Mars! January will be an excellent opportunity to spot this planet and some of its details with a medium-sized telescope. Be sure to catch these three events this month.

Martian Retrograde

Mars entered retrograde (or backward movement relative to its usual direction) on December 7, 2024, and will continue throughout January into February 23, 2025. You can track the planet’s progress by sketching or photographing Mars’ position relative to nearby stars. Be consistent with your observations, taking them every few nights or so as the weather permits. You can use free software like Stellarium or Stellarium Web (the browser version) to help you navigate the night as Mars treks around the sky. You can find Mars above the eastern horizon after 8:00 PM local time.

A star chart depicting the path of Mars through the constellations Gemini and Cancer over several months. The path of Mars is marked with an orange line and labeled with specific dates (e.g., Sept. 1, 2024, Nov. 1, 2024, Feb. 1, 2025, Jun. 1, 2025). The background includes constellations such as Cancer, Gemini, and Orion, labeled with star names like Betelgeuse, Rigel, Pollux, and Procyon. Jupiter is also visible in the upper right. The chart shows Mars’ apparent retrograde motion as it loops and crosses its previous path.
This mid-January chart shows the path of Mars from September 2024 to June 2025 as it enters and then exits in retrograde motion. Mars appears to change its direction of motion in the sky because Earth is passing the slower-moving Mars in its orbit.
Stellarium

Hide and Seek

On the night of January 13th, you can watch Mars ‘disappear’ behind the Moon during an occultation. An occultation is when one celestial object passes directly in front of another, hiding the background object from view. This can happen with planets and stars in our night sky, depending on the orbit of an object and where you are on Earth, similar to eclipses.

A detailed image of the Full Moon dominating the frame against a black night sky. Below the lower-left edge of the Moon, Mars appears as a small, bright reddish-orange dot, partially hidden as it undergoes an occultation by the Moon. The Moon's surface is detailed with visible craters and maria.
A simulated view of the Moon as Mars begins its occultation on January 13, 2025.
Stellarium

Depending on where you are within the contiguous United States, you can watch this event with the naked eye, binoculars, or a small telescope. The occultation will happen for over an hour in some parts of the US. You can use websites like Stellarium Web or the Astronomical League’s ‘Moon Occults Mars’ chart to calculate the best time to see this event.

Closer and Closer

As you observe Mars this month to track its retrograde movement, you will notice that it will increase in brightness. This is because Mars will reach opposition by the evening of January 16th. Opposition happens when a planet is directly opposite the Sun, as seen from Earth. You don’t need to be in any specific city to observe this event; you only need clear skies to observe that it gets brighter. It’s also when Mars is closest to Earth, so you’ll see more details in a telescope.

Want a quick and easy way to illustrate what opposition is for Jupiter, Saturn, Mars, or other outer worlds? Follow the instructions on our Toolkit Hack: Illustrating Opposition with Exploring the Solar System page using our Exploring Our Solar System activity!

A full globe view of reddish Mars featuring Valles Marineris - which looks like a huge gash on the planet.
A mosaic of the Valles Marineris hemisphere of Mars projected into point perspective, a view similar to that which one would see from a spacecraft. The mosaic is composed of 102 Viking Orbiter images of Mars.
NASA/JPL-Caltech

Mars has fascinated humanity for centuries, with its earliest recorded observations dating back to the Bronze Age. By the 17th century, astronomers were able to identify features of the Martian surface, such as its ice caps and darker regions. Since the 1960s, exploration of the Red Planet has intensified with robotic missions from various space organizations. Currently, NASA has five active missions, including rovers and orbiters, with the future focused on human exploration and habitation. Mars will always fill us with a sense of wonder and adventure as we reach for its soil through initiatives such as the Moon to Mars Architecture and the Mars Sample Return campaign.

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Astronomy Activation Ambassadors: A New Era

Astronomy Activation Ambassadors: A New Era

3 min read

Astronomy Activation Ambassadors: A New Era

The NASA Science Activation Program’s Astronomy Activation Ambassadors (AAA) project aims to measurably enhance student Science, Technology, Engineering, and Mathematics (STEM) engagement via middle school, high school, and community college science teacher professional development.

In 2024, AAA transitioned its focus to the development of an Astronomy Academy with varying levels of extent and intensity available to more than 300 teachers per year. Participants draw on NASA resources and Subject Matter Experts (SME) to enhance their teaching and help share their excitement about astronomy with their students. The three strands that comprise the Astronomy Academy are:

  1. webinars regarding NASA astrophysics and planetary science content and facilities,
  2. curriculum workshops enabling classroom use of an electromagnetic spectrum and multi-wavelength astronomy (EMS/MWA) curriculum, and
  3. STEM immersion experiences including guided visits to working observatories.

The first two of the AAA program’s new type of STEM immersion experiences took place in June and September, 2024. During the weekend of June 22-23, 19 teachers gathered in San Jose, California for a full agenda, including:

  • NASA SME presentations regarding planetary protection and exoplanet detection,
  • a journey to the University of California’s Lick Observatory on nearby Mt. Hamilton for an in-depth guided tour of the observatory’s astronomy research facilities, which included engagement with the astronomers using the 3-meter Shane telescope, and
  • a 4-hour hands-on EMS/MWA curriculum teaching workshop.

A similar STEM immersion sequence was offered September 14-15 to 23 AAA teachers who attended a curriculum teaching workshop, learned about current infrared astronomy research from NASA Jet Propulsion Laboratory scientists, and received guided visits to the Keck Observatory’s remote observing facility on the Caltech campus and the Mt. Wilson Observatory, including a half-night’s reserved use of the historic Mt. Wilson 60-inch telescope. The teachers were invited to submit a list of objects to be observed with the Mt. Wilson telescope and viewed a wonderful array of star clusters, colorful double stars, and galaxies, with a grand finale view of Saturn and its rings.

Teacher participant, Domina Stamas (Westlake Charter School, Sacramento, California), had this to say: “My students and I are already benefiting greatly from the combination of NASA resources, science content, and curricular materials we have received from the AAA project. The evening at Lick Observatory talking with the astronomers who were using the research telescopes watching the laser guide star setup in action was a rich experience. I can convey to my students how scientists actually practice their craft.”

The Astronomy Activation Ambassador project’s efforts to improve student STEM learning and engagement via science teacher professional development are detailed at: https://www.seti.org/aaa

Educator enrollment is still open via the participant registration form:
https://forms.gle/G34vCzz63ko5RRrM8

The AAA project, led by the SETI Institute, is supported by NASA under cooperative agreement award number NNX16AC51A and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn

Group of 23 teachers standing in a closed observatory dome in front of a long telescope on top of a support column.
June 2024 teacher participants in front of the Lick Observatory’s historic 36-inch refracting telescope.
SETI Institute/C. Clark

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Last Updated
Dec 31, 2024
Editor
NASA Science Editorial Team
Location
Jet Propulsion Laboratory

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Red and Green Aurora Move Through Earth’s Atmosphere

Red and Green Aurora Move Through Earth’s Atmosphere

iss072e031823 (Oct. 7, 2024) -- Peering through the window of the SpaceX Dragon Endeavour spacecraft, NASA astronaut Matthew Dominick captured this image of the SpaceX Dragon Freedom spacecraft as vivid green and pink aurora swirled through Earth's atmosphere while the International Space Station soared 273 miles above the Indian Ocean.

Peering through the window of the SpaceX Dragon Endeavour spacecraft, NASA astronaut Matthew Dominick captured this image on Oct. 7, 2024 of the SpaceX Dragon Freedom spacecraft as vivid green and pink aurora swirled through Earth’s atmosphere while the International Space Station soared 273 miles above the Indian Ocean.

Visit Dominick’s photography on station to experience the wonders of space through his eyes, enriched by his remarkable journey of orbiting the Earth 3,760 times.

To see a short-term forecast of the location and intensity of the next aurora check this link: Aurora – 30 Minute Forecast and also NASA’s Guide to Finding and Photographing Auroras.

Image Credit: NASA/Matthew Dominick

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Gary Daines

Assessment of PFO as Related to DCS in the Spaceflight Environment and During Ground Testing

Assessment of PFO as Related to DCS in the Spaceflight Environment and During Ground Testing

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

PFO, OCHMO
In-person participants L-R standing: Dave Francisco, Joanne Kaouk, Dr. Richard Moon, Dr. Tony Alleman, Dr. Sean Hardy, Sarah Childress, Kristin Coffey, Dr. Ed Powers, Dr. Doug Ebersole, Dr. Steven Laurie, Dr. Doug Ebert; L-R seated: Dr. Alejandro Garbino, Dr. Robert Sanders, Dr. Kristi Ray, Dr. Mike Gernhardt, Dr. Joseph Dervay, Dr. Matt Makowski). Not pictured: Dr. Caroline Fife

In June 2024, the NASA Office of the Chief Health and Medical Officer (OCHMO) Standards Team hosted an independent assessment working group to review the status and progress of research and clinical activities intended to mitigate the risk of decompression sickness (DCS) related to patent foramen ovale (PFO) during spaceflight and associated ground testing and human subject studies.

Decompression sickness (DCS) is a condition which results from dissolved gases (primarily nitrogen) forming bubbles in the bloodstream and tissues. It is usually experienced in conditions where there are rapid decreases in ambient pressure, such as in scuba divers, high-altitude aviation, or other pressurized environments. The evolved gas bubbles have various physiological effects and can obstruct the blood vessels, trigger inflammation, and damage tissue, resulting in symptoms of DCS. NASA presently classifies DCS into two categories: Type I DCS, which is less severe, typically leads to musculoskeletal symptoms including pain in the joints or muscles, or skin rash. Type II DCS is more severe and commonly results in neurological, inner ear, and cardiopulmonary symptoms. The risk of DCS in spaceflight presents during extravehicular activities (EVAs) in which astronauts perform mission tasks outside the spaceflight vehicle while wearing a pressurized suit at a lower pressure than the cabin pressure. DCS mitigation protocols based on strategies to reduce systemic nitrogen load are implemented through the combination of habitat environmental parameters, EVA suit pressure, and breathing gas procedures (prebreathe protocols) to achieve safe and effective mission operations. The pathophysiology of DCS has still not been fully elucidated since cases occur despite the absence of detected gas bubbles but includes right to left shunting of venous gas emboli (VGE) via several potential mechanisms, one of which is a Patent Foramen Ovale (PFO).

Decompression sickness (DCS): Bubbles form in blood and tissue which causes local damage.
Arterial gas embolism (AGE): Results from bubbles entering the bloodstream and blocking blood flow which can cause tissue damage.
Peter N. Schochet, MD and Hauw S. Lie, MD

From: Dr. Schochet & Dr. Lie, Pediatric Pulmonologists

Reference OCHMO-TB-037 Decompression Sickness (DCS) Risk Mitigation technical brief for additional information.

A PFO is a shunt between the right atrium and the left atrium of the heart, which is a persisting remnant of a physiological communication present in the fetal heart. Post-natal increases in left atrial pressure usually force the inter-septal valve against the septum secundum and within the first 2 years of life, the septae permanently fuse due to the development of fibrous adhesions. Thus, all humans are born with a PFO and approximately 75% of PFOs fuse following childbirth. For the 25% of the population’s whose PFOs do not fuse, ~6% have what is considered by some to be a large PFO (> 2 mm). PFO diameter can increase with age. The concern with PFOs is that with a right to left shunt between the atria, venous emboli gas may pass from the right atrium (venous) to the left atrium (arterial) (“shunt”), thus by-passing the normal lung filtration of venous emboli which prevent passage to the arterial system. Without filtration, bubbles in the arterial system may lead to a neurological event such as a stroke. Any activity that increases the right atrium/venous pressure over the left atrium/arterial pressure (such as a Valsalva maneuver, abdominal compression) may further enable blood and/or emboli across a PFO/shunt.

Patent foramen ovale (PFO), a hole between the left and right atria of the heart, is known to be a cause of stroke in young adults.
S. Mazzucco, L. Li, L. Binney, P.M. Rothwell

From: Nuffield Department of Clinical Neurosciences

The purpose of this working group was to review and provide analysis on the status and progress of research and clinical activities intended to mitigate the risk of PFO and DCS issues during spaceflight. Identified cases of DCS during NASA exploration atmosphere ground testing conducted in pressurized chambers led to the prioritization of the given topic for external review. The main goals of the working group included:

  1. Quantification of any increased risk associated with the presence of a PFO during decompression protocols utilized in ground testing and spaceflight EVAs, as well as unplanned decompressions (e.g., cabin depressurization, EVA suit leak).
  2. Describe risks and benefits of PFO screening in astronaut candidates, current crewmembers, and chamber test subjects.
  3. What are potential risk reduction measures that could be considered if a person was believed to be at increased risk of DCS due to a PFO?
  4. What research and/or technology development is recommended that could help inform and/or mitigate PFO-related DCS risk?

The working group took place over two days at NASA’s Johnson Space Center and included NASA subject matter experts and stakeholders, as well as invited external reviewers from areas including cardiology, hypobaric medicine, spaceflight medicine, and military occupational health. During the working group, participants were asked to review past reports and evidence related to PFOs and risk of DCS, materials and information regarding NASA’s current experience and practices, and case studies and subsequent decision-making processes. The working group culminated in an open-forum discussion where recommendations for current and future practices were conferred and subsequently summarized in a final summary report, available on the public NASA OCHMO Standards Team website.

The following key findings are the main take-aways from the OCHMO independent assessment:

  1. In an extreme exposure/high-risk scenario, excluding individuals with a PFO and treating PFOs does not necessarily decrease the risk of DCS or create a ‘safe’ environment. It may create incremental differences and slightly reduce overall risk but does not make the risk zero. There are other physiological factors that also contribute to the risk of DCS that may have a larger impact (see 7.0 Other Physiological Factors in the findings section). 
  2. Based on the available evidence and the risk of current decompression exposures (based on current NASA protocols and NASA-STD-3001 requirements to limit the risk of DCS), it is not recommended to screen for PFOs in any spaceflight or ground testing participants. The best strategy to reduce the risk of DCS is to create as safe an environment as possible in every scenario, through effective prebreathe protocols, safety, and the capability to rapidly treat DCS should symptoms occur. 
  3. Based on opinion, no specific research is required at this time to further characterize PFOs with DCS and altitude exposure, due to the low risk and preference to institute adequate safe protocols and ensuring treatment availability both on the ground and in spaceflight.
  4. For engineering protocols conducted on the ground, it should be ensured that the same level of treatment capability (treatment chamber in the immediate vicinity of the testing) is provided as during research protocols. The ability to immediately treat a DCS case is critical in ensuring the safety of the test subjects.

The full summary report includes detailed background information, discussion points from the working group, and conclusions and recommendations. The findings from the working group and resulting summary report will help to inform key stakeholders in decision-making processes for future ground testing and spaceflight operations with the main goal of protecting crew health and safety to ensure overall mission success.

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Sarah D. Childress

Sarah D. Childress

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Sarah D. Childress