Spaceweather.com Time Machine

13 min read Original article ↗
 

Solar wind
speed: 430.7 km/sec
density: 1.13 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 1147 UT

X-ray Solar Flares
6-hr max: C1
2206 UT May04
24-hr: M1
0133 UT May04
explanation | more data
Updated: Today at: 2350 UT

Daily Sun: 04 May 26
Expand: labels | no labels
All of these sunspots have stable magnetic fields unlikely to produce strong solar flares. Credit: NASA/SDO

Sunspot number: 138
What is the sunspot number?
Updated 04 May 2026

Current Auroral Oval:

Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation

Planetary K-index
Now: Kp= 6.33 storm
24-hr max: Kp= 6.33
storm
explanation | more data

Interplanetary Mag. Field
Btotal: 11.36 nT
Bz: -7.05 nT south
more data: ACE, DSCOVR
Updated: Today at 1147 UT

Coronal Holes: 04 May 26


Solar wind flowing from this minor coronal hole will reach Earth on May 7th. It is unlikely to cause geomagnetic storms.
Credit: NASA/SDO | more data

Spotless Days
Current Stretch: 0 days
2026 total: 3 days (2%)
2025 total: 0 days (0%)
2024 total: 0 days (0%)
2023 total: 0 days (0%)
2022 total: 1 day (<1%)
2021 total: 64 days (18%)
2020 total: 208 days (57%)
2019 total: 281 days (77%)
2018 total: 221 days (61%)
2017 total: 104 days (28%)
2016 total: 32 days (9%)
2015 total: 0 days (0%)
2014 total: 1 day (<1%)
2013 total: 0 days (0%)
2012 total: 0 days (0%)
2011 total: 2 days (<1%)
2010 total: 51 days (14%)
2009 total: 260 days (71%)
2008 total: 268 days (73%)
2007 total: 152 days (42%)
2006 total: 70 days (19%)

Updated 04 May 2026
Thermosphere Climate Index
today: 17.03x1010 W Neutral
Max: 49.4
x1010 W Hot (10/1957)
Min: 2.05
x1010 W Cold (02/2009)
explanation | more data: gfx, txt
Updated 04 May 2026

The Radio Sun
10.7 cm flux: 143 sfu
explanation | more data
Updated 04 May 2026

Cosmic Rays Solar Cycle 25 is near its peak, and this is reflected in the number of cosmic rays entering Earth's atmosphere. Neutron counts from the University of Oulu's Sodankyla Geophysical Observatory show that cosmic rays reaching Earth are slowly declining--a result of the yin-yang relationship between the solar cycle and cosmic rays.

Oulu Neutron Counts

Percentages of the Space Age average:
today: -7.2% Low
48-hr change: -0.2%
Max: +11.7% Very High
(12/2009)
Min: -32.1% Very Low (06/1991)
explanation | more data
Updated 24 Mar 2026 @ 0700 UT


SPACE WEATHER
NOAA Forecasts

Updated at: 2026 May 04 2200 UTC

FLARE

0-24 hr

24-48 hr

CLASS M

30 %

30 %

CLASS X

05 %

05 %

Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm

Updated at: 2026 May 04 2200 UTC

Mid-latitudes

0-24 hr

24-48 hr

ACTIVE

40 %

20 %

MINOR

20 %

05 %

SEVERE

05 %

01 %

High latitudes

0-24 hr

24-48 hr

ACTIVE

10 %

15 %

MINOR

30 %

25 %

SEVERE

50 %

25 %

 

Monday, May. 4, 2026

What's up in space
       
 

This is an AI Free Zone: AI is everywhere -- except here. Spaceweather.com is written by Dr. Tony Phillips, a carbon-based lifeform with 30 yrs of forecasting experience. If you find a mistake, rest assured it was made by a real human being.

 

METEORS FROM HALLEY'S COMET: Earth is entering a stream of debris from Halley's Comet, source of the annual eta Aquarid meteor shower. Forecasters expect the shower to peak on May 5th and 6th. Rates could be as high as 30 meteors per hour in the southern hemisphere, but only half that in the northern hemisphere. The best time to look is just before local sunrise when the constellation Aquarius is high in the sky. Free: Space Weather Newsletter

ARE WE OVERDUE FOR A SUPERFLARE? We've all heard of X-class solar flares--powerful explosions on the sun that pepper satellites with energetic particles and trigger great geomagnetic storms. They can be scary. But not as scary as a new category of solar flare being discussed by researchers: the "S-flare"--a solar superflare stronger than X10.

A new paper published in the Journal of Geophysical Research suggests we may be overdue for one.

During the current solar cycle, Solar Cycle 25, Earth has not yet experienced an S-flare. That's a little unusual, according to researchers led by V.M. Velasco Herrera of the National Autonomous University of Mexico. The team looked at 50 years of data from Earth-orbiting satellites. Among 95,627 solar flares, they found 37 Earth-directed S-flares. Every solar cycle since the 1970s has produced one--except Solar Cycle 25.

There are some clues to when the next S-flare might happen. In the 50-year dataset, the researchers found two underlying rhythms: 1.7 years and 7 years, both linked to magneto-Rossby waves inside the sun. When both rhythms swing into their positive phase at the same time, the probability of an S-flare spikes.

Right: An S-class solar flare (X45) on Nov. 4, 2003. [more]

According to those rhythms, we're exiting a high-risk S-flare window now: mid-2025 through mid-2026. The next high-risk window opens in early 2027 and lasts about 6 months.

In May 2024, Europe's Solar Orbiter detected two possible S-flares on the farside of the sun. Their intensity (with significant error bars) was X11.1 and X16.5. The sun fired the gun; we just happened to be standing behind the target.

Maybe next time. Stay tuned for updates as the 2027 window approaches.

Realtime Space Weather Photo Gallery
Free:
Spaceweather.com Newsletter

MOTHER'S DAY IS THIS SUNDAY: Are you looking for an out-of-this world Mother's Day gift? Consider this: Every time the students of Earth to Sky Calculus launch a cosmic ray balloon, they include something extra in the payload--something Mom will love:

Every item in the Earth to Sky Store has flown to the edge of space and comes with a greeting card showing the item in flight. The interior of the card tells the story of the gift's journey from launch to landing. Mom-satisfaction guaranteed!

Far Out Gifts: Earth to Sky Store
All sales support hands-on STEM education

AIRGLOW DUNES (UPDATED): You may have heard of "aurora dunes" -- a recently identified form of Northern Lights named after their resemblence to ripples in desert sand. Researchers led by Minna Palmroth (University of Helsinki) first explained them in a paper published only a few years ago.

Now, let us introduce you to "airglow dunes":

Zdenek Bardon took this picture from the European Southern Observatory in Paranal, Chile, on April 17th. "I was photographing the Milky Way and caught some rippling green airglow at the same time."

The dunes are a "mesospheric bore," a type of atmospheric gravity wave that springs up from Earth's surface and gets caught in a thermal waveguide ~100 km high. Although auroras and airglow are formed in completely different ways (solar activity vs. terrestrial photochemistry) mesospheric bores can modulate them both.

Update: Space scientist Steven M. Smith of Boston University has a different interpretation of these dunes. "They are more likely to be ripples due to a Kelvin-Helmholtz instability," he believes. "This kind of instability is caused by vertical shears in wind speed, which are common in the mesosphere. The effect is also seen on the bottom of sandy streams - the wave-like undulations in the sand on the bottom is due to the rapid change in velocity of the water."

Smith prefers Kelvin-Helmholtz over bores in part because "a bore is much more extensive with the wave-fronts extending across the entire sky."

Realtime Airglow Photo Gallery
Free:
Spaceweather.com Newsletter


Realtime Aurora Photo Gallery
Free:
Spaceweather.com Newsletter


Every night, a network of NASA all-sky cameras scans the skies above the United States for meteoritic fireballs. Automated software maintained by NASA's Meteoroid Environment Office calculates their orbits, velocity, penetration depth in Earth's atmosphere and many other characteristics. Daily results are presented here on Spaceweather.com.

On May 4, 2026, the network reported 1 fireballs.
(1 sporadic)

In this diagram of the inner solar system, all of the fireball orbits intersect at a single point--Earth. The orbits are color-coded by velocity, from slow (red) to fast (blue). [Larger image] [movies]

Potentially Hazardous Asteroids (PHAs) are space rocks larger than approximately 100m that can come closer to Earth than 0.05 AU. None of the known PHAs is on a collision course with our planet, although astronomers are finding new ones all the time.

On May 4, 2026 there were 2349 potentially hazardous asteroids.

Recent & Upcoming Earth-asteroid encounters:

Asteroid

Date(UT)

Miss Distance

Velocity (km/s)

Diameter (m)

2026 HP3

2026-Apr-29

15.5 LD

11.3

29

2026 HL3

2026-Apr-29

6.7 LD

8.6

25

2026 HX3

2026-May-01

8.1 LD

11.4

21

2026 HY3

2026-May-01

7.2 LD

9

18

2026 HZ3

2026-May-01

4 LD

8.4

31

2026 GW3

2026-May-02

13.9 LD

5.8

21

2026 HM6

2026-May-02

3.8 LD

18.4

14

2026 HA3

2026-May-02

5.1 LD

12.1

48

2026 HD3

2026-May-02

8.4 LD

11.5

20

2026 HL6

2026-May-02

6.2 LD

20.6

23

2026 JA

2026-May-03

1.1 LD

11.8

15

2026 HE2

2026-May-03

15.5 LD

6.6

24

2026 GD1

2026-May-03

14.6 LD

6.6

48

2026 HK4

2026-May-05

11 LD

20.3

23

2026 HN1

2026-May-06

9.2 LD

14.2

66

2026 HA4

2026-May-07

4.1 LD

9

19

2026 HY2

2026-May-07

5 LD

9

33

2026 HD2

2026-May-08

17.7 LD

10.7

43

2020 GE3

2026-May-09

11.1 LD

5.9

21

2023 VR5

2026-May-16

7.5 LD

2.3

10

2026 HC5

2026-May-17

7.1 LD

6.7

21

2025 KR4

2026-May-18

15.2 LD

5.9

22

2023 KH4

2026-May-24

5.5 LD

7.9

14

2023 KZ1

2026-May-24

9 LD

13.4

20

2026 HW2

2026-May-29

17.7 LD

12.5

127

2023 BM4

2026-May-30

12.2 LD

5.7

64

2021 KN2

2026-Jun-03

8.9 LD

8.9

7

2018 GE

2026-Jun-07

16.4 LD

3.1

11

2016 VS

2026-Jun-12

20 LD

11.1

12

530520

2026-Jun-12

16.1 LD

14.6

152

2003 LN6

2026-Jun-18

3.7 LD

3.9

41

2025 WC4

2026-Jun-21

10.2 LD

19.2

304

2015 LM24

2026-Jun-22

18.2 LD

13.8

71

152637

2026-Jun-27

6.7 LD

8.9

947

Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU.

  Cosmic Rays in the Atmosphere

SPACE WEATHER BALLOON DATA: Almost once a week, Spaceweather.com and the students of Earth to Sky Calculus fly space weather balloons to the stratosphere over California. These balloons are equipped with sensors that detect secondary cosmic rays, a form of radiation from space that can penetrate all the way down to Earth's surface. Our monitoring program has been underway without interruption for 10 years, resulting in a unique dataset of in situ atmospheric measurements.

Latest results (Nov. 2024): Atmospheric radiation is sharply decreasing in 2024. Our latest measurements in November registered a 10-year low:

What's going on? Ironically, the radiation drop is caused by increasing solar activity. Solar Cycle 25 has roared to life faster than forecasters expected. The sun's strengthening and increasingly tangled magnetic field repels cosmic rays from deep space. In addition, solar coronal mass ejections (CMEs) sweep aside cosmic rays, causing sharp reductions called "Forbush Decreases." The two effects blend together to bring daily radiation levels down.

.Who cares? Cosmic rays are a surprisingly "down to Earth" form of space weather. They can alter the chemistry of the atmosphere, trigger lightning, and penetrate commercial airplanes. According to a study from the Harvard T.H. Chan school of public health, crews of aircraft have higher rates of cancer than the general population. The researchers listed cosmic rays, irregular sleep habits, and chemical contaminants as leading risk factors. A number of controversial studies (#1, #2, #3, #4) go even further, linking cosmic rays with cardiac arrhythmias and sudden cardiac death.

Technical notes: The radiation sensors onboard our helium balloons detect X-rays and gamma-rays in the energy range 10 keV to 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

Data points in the graph labeled "Stratospheric Radiation" correspond to the peak of the Regener-Pfotzer maximum, which lies about 67,000 feet above central California. When cosmic rays crash into Earth's atmosphere, they produce a spray of secondary particles that is most intense at the entrance to the stratosphere. Physicists Eric Regener and Georg Pfotzer discovered the maximum using balloons in the 1930s and it is what we are measuring today.

  The official U.S. government space weather bureau

  The first place to look for information about sundogs, pillars, rainbows and related phenomena.

  Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever.

  3D views of the sun from NASA's Solar and Terrestrial Relations Observatory

  Realtime and archival images of the Sun from SOHO.

  information about sunspots based on the latest NOAA/USAF Active Region Summary

  current counts of failed and deployed Starlink satellites from Jonathan's Space Page. See also, all satellite statistics.

  Authoritative predictions of space junk and satellite re-entries

  from the NOAA Space Environment Center

  fun to read, but should be taken with a grain of salt! Forecasts looking ahead more than a few days are often wrong.

  from the NOAA Space Environment Center

  the underlying science of space weather

Got a chipped or cracked windshield that prevents you from seeing space weather events while driving? Get windshield replacement from SR Windows & Glass with free mobile auto glass service anywhere in the Phoenix area.

  These links help Spaceweather.com stay online. Thank you to our supporters!

 


T CrB NOVA WATCH
today: m=10.3 (May 4.5)
yesterday: m=10.2

AAVSO data: #1, #2.

Explanation: When the nova explodes, the visual magnitude of the star will jump from +10 (invisible to the naked eye) to +2 (about as bright as the North Star).


Starlink Statistics
Total Launched: 11,973
In orbit:
10,392
Updated: 04 May 2026

Starlink Re-entries (2026)
January: 24
February: 54
March: 48
April: 51
May: 2 so far
Updated: 04 May 2026

Starlink Re-entries (yearly)
2020 total:
46
2021 total:
78
2022 total:
100
2023 total: 88
2024 total: 308
2025 total: 657
2026 total: 178 so far

Data sources: #1, #2, #3; Histograms: launches, reentries



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