diff --git a/Time-Stepping Naked Planet Model/Grading/GWmod1.py b/Time-Stepping Naked Planet Model/Grading/GWmod1.py
new file mode 100644
index 0000000..90356e0
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+++ b/Time-Stepping Naked Planet Model/Grading/GWmod1.py	
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+#My first tijme making a plot for climate modeling.
+#Hopefully, this works.
+#Note that using spreadsheets for this course is optional;
+#the only way to get credit is with Python3!
+
+"""The background for this material can be found in Sections 2 and 3 of Part I
+of this class. Joules are units of energy; Watts are energy flow (J/s).
+The temperature of a planet is determined by balancing energy fluxes in and out of a planet.
+Incoming solar heat is determined by L*(1-albedo)/4,
+and outgoing infrared is calculated as epsilon * sigma * T^4."""
+
+"""The heat capacity of the surface planet depends on the water thickness.
+Using the fact that 1 gram of water warms by 1 K with a 4.2J (1 cal) of heat,
+and the density of water, to calculate how many Joules of energy it takes
+to raise the temperature of 1 m2 of the surface, given some water depth
+in meters."""
+
+"""The goal is to numerically simulate how the planetary temperature of a
+naked planet would change through time as it approaches equilibrium
+(the state at which it stops changing, which we calculated before).
+The planet starts with some initial temperature.
+The “heat capacity” (units of Joules / m2 K) of the planet is set by
+a layer of water which absorbs heat and changes its temperature.
+If the layer is very thick, it takes a lot more heat (Joules) to change the temperature.
+The differential equation you are going to solve is:"""
+#d(HeatContent)/dt = L*(1-alpha)/4 - epsilon * sigma * T^4
+"where the heat content is related to the temperature by the heat capacity:"
+#T[K] = HeatContent [J/m2] / HeatCapacity [J/m2 K]
+"""The numerical method is to take time steps, extrapolating the heat content
+from one step to the next using the incoming and outgoing heat fluxes,
+same as you would balance a bank account by adding all the income and subtracting all the expenditures
+over some time interval like a month.
+The heat content "jumps" from the value at the beginning of the time step,
+to the value at the end, by following the equation:"""
+#HeatContent(t+1) = HeatContent(t) + dHeatContent/dT * TimeStep
+"""This scheme only works if the time step is short enough so that
+nothing too huge happens through the course of the time step.
+Set the model up with the following constants:"""
+timeStep = 40           # years; convert to seconds.
+time = 0                 # years; this shall denote how much time has passed in total.
+T = 0                    # Kelvin, according to question demands.
+waterDepth = 2000        # meters; multiply by cH2O and water density.
+L = 1350                 # W m-2, same as J s-1 m-2 (Solar Constant) -> multiply by no. of seconds in each timestep
+albedo = 0.3             # alpha
+epsilon = 1
+sigma = 5.67E-8          # W m-2 K-4
+cH2O = 4200              # specific heat capacity of water (units of 4200 J kg-1 K-1).
+rhoH2O = 1000            # Density is 1000 kg m-3.
+energy_per_m2 = waterDepth * cH2O * rhoH2O #in J m-2 K-1
+#heat influx and outflux must be calculated along the way.
+import numpy
+import matplotlib.pyplot
+#Getting our lists needed with the very first variables already in:
+nSteps = input("Please use 20 or more")
+#apparently the autograder that the MOOC uses also mistakes strings for operators.
+nSteps = int(nSteps)
+time_list = [time]
+temperature_list = [T]
+HeatContent = 0 #only true when T = 0 Kelvin, this is the heat content of the Earth.
+difference = 0
+outflux = 0
+for x in range(nSteps):
+    time = time + timeStep
+    time_list.append(time)
+    difference = (L * (1 - albedo) / 4 - (epsilon * sigma * T**4)) #W m-2
+    HeatContent = HeatContent + difference * 365 * 24 * 60 * 60 * timeStep #J m-2
+    T = (HeatContent / energy_per_m2) #Kelvin
+    outflux = epsilon * sigma * T**4 # as per instructions
+    temperature_list.append(T)
+#derive answers and end with:
+matplotlib.pyplot.plot(time_list, temperature_list)
+matplotlib.pyplot.show()
+#Give the last temperature derived by the model:
+#print(temperature_list[-1], outflux)
+#The tolerances in the grader for temperatures are 2-3 degrees C,
+#and for the heat fluxes, +- 0.1 W/m2.
diff --git a/Time-Stepping Naked Planet Model/Grading/Naked_Earth.py b/Time-Stepping Naked Planet Model/Grading/Naked_Earth.py
new file mode 100644
index 0000000..8a63aea
--- /dev/null
+++ b/Time-Stepping Naked Planet Model/Grading/Naked_Earth.py	
@@ -0,0 +1,32 @@
+import matplotlib.pyplot as plt
+
+timeStep = 10           # years
+waterDepth = 4000        # meters
+L = 1350                 # Watts/m2
+albedo = 0.3
+epsilon = 1
+sigma = 5.67E-8          # W/m2 K4
+#nSteps = int(input(""))
+nSteps=200
+
+heat_cap=waterDepth*4.2E6 #J/Kg/deg
+time_list=[0]
+temperature_list=[400]
+heat_content=heat_cap*temperature_list[0]
+heat_in=L*(1-albedo)/4
+heat_out=0
+secs_in_yr=3.14E7
+
+for t in range(0,nSteps):
+    time_list.append(timeStep+time_list[-1])
+    heat_out=epsilon*sigma*pow(temperature_list[-1],4)
+    heat_content=heat_content+(heat_in-heat_out)*timeStep*secs_in_yr
+    temperature_list.append(heat_content/heat_cap)
+    heat_out = epsilon * sigma * pow(temperature_list[-1], 4)
+print(temperature_list[-1])
+#print(temperature_list[-1], heat_out)
+plt.plot(time_list, temperature_list, marker='.', color="k")
+plt.xlabel("Time (years)")
+plt.ylabel("Temperature (degrees Kelvin)")
+plt.show()
+
diff --git a/Time-Stepping Naked Planet Model/Grading/naked_planet_tosubmit.py b/Time-Stepping Naked Planet Model/Grading/naked_planet_tosubmit.py
new file mode 100644
index 0000000..4d567f2
--- /dev/null
+++ b/Time-Stepping Naked Planet Model/Grading/naked_planet_tosubmit.py	
@@ -0,0 +1,68 @@
+# %%
+
+
+# %%
+import numpy as np
+import matplotlib.pyplot as plt 
+
+# Set up constants as given:
+timeStep_years = 100           # years
+waterDepth = 4000              # meters
+L = 1350                       # W/m²
+albedo = 0.3
+epsilon = 1
+sigma = 5.67e-8                # W/m² K^4
+
+# The incoming solar flux is constant:
+incoming_flux = L * (1 - albedo) / 4   # W/m²
+
+# Calculate the heat capacity (J/m² K)
+# (water density = 1000 kg/m³, specific heat = 4184 J/(kg·K))
+heat_capacity = waterDepth * 1000 * 4184
+
+# Read the number of time steps from stdin
+nSteps = int(input(""))
+
+# Set the initial conditions.
+# (Initial temperature is chosen in Kelvins; 0 K is allowed though not physical.)
+initial_temperature = 0.0  # Kelvin
+heatContent = initial_temperature * heat_capacity  # in J/m²
+
+# Prepare lists for time and temperature (for plotting, if desired)
+time_list = [0]
+temperature_list = [initial_temperature]
+
+# Convert the time step to seconds.
+dt = timeStep_years * 365 * 24 * 3600
+
+# Integration loop: update heat content and temperature each step.
+for i in range(nSteps):
+    # Current temperature in Kelvin:
+    T = heatContent / heat_capacity
+    
+    # Differential equation: dHeat/dt = incoming_flux - ε·σ·(T)⁴
+    dH_dt = incoming_flux - epsilon * sigma * (T**4)
+    
+    # Update the heat content over the time step:
+    heatContent = heatContent + dH_dt * dt
+    
+    # Append new time and temperature to lists:
+    time_list.append((i+1) * timeStep_years)
+    temperature_list.append(heatContent / heat_capacity)
+
+# Compute the final temperature (in Kelvin) and the corresponding outgoing heat flux.
+final_temperature = heatContent / heat_capacity
+final_heat_flux = epsilon * sigma * (final_temperature**4)
+
+# Output only the final temperature and heat flux.
+print(final_temperature, final_heat_flux)
+
+# Plotting code
+plt.plot(time_list, temperature_list)
+plt.show()
+
+
+# %%
+
+
+
diff --git a/Time-Stepping Naked Planet Model/naked_planet.py b/Time-Stepping Naked Planet Model/naked_planet.py
new file mode 100644
index 0000000..66cce23
--- /dev/null
+++ b/Time-Stepping Naked Planet Model/naked_planet.py	
@@ -0,0 +1,51 @@
+import numpy
+import matplotlib.pyplot
+
+
+# Inputs
+timeDuration = 2000                    # years
+timeStep = 10                          # years
+waterDepth = 4000                          # meters
+initialTemp = 400
+
+# Constants
+secondToYear = 60*60*24*365
+specificWaterHeatCapacity  = 4.2E3      # kg/m^3
+waterDensity = 1000                     # J/kg*m^3
+L = 1350                                # Watts/m2
+albedo = 0.3
+epsilon = 1
+sigma = 5.67E-8                         # W/m2 K4
+
+
+# Calc amount of steps for given duration and resolution
+nSteps = int(timeDuration/timeStep)
+
+initialHeat = initialTemp * (waterDepth*waterDensity*specificWaterHeatCapacity)
+initialRadiatedHeat = epsilon * sigma * pow(initialTemp,4)
+T = [initialTemp]               # K
+Q = [initialHeat]               # Watt/m^2
+time = [0]                      # years
+heatOut = [initialRadiatedHeat] # Watt/m^2
+# print(initialRadiatedHeat)
+
+for i in range(nSteps):
+    # Calculate the heat change rate 
+    dQ_dt = (L * (1 - albedo)/4) - epsilon * sigma * pow(T[-1],4)
+    # Add heat change over step period to total heat in system   
+    Q.append(Q[-1] + dQ_dt * timeStep * secondToYear)
+    # Calculate temperature of planet based on heat in system
+    T.append(Q[-1] / (waterDepth*waterDensity*specificWaterHeatCapacity))
+    # Calculate only the outgoing heat
+    heatOut.append(epsilon * sigma * pow(T[-1],4)) 
+    # Save timestep for plotting
+    time.append(time[-1] + timeStep)
+
+print(T[-1])
+
+
+matplotlib.pyplot.plot(time, T)
+matplotlib.pyplot.title("Time-dependent temperature of a naked planet")
+matplotlib.pyplot.xlabel('Time (years)')
+matplotlib.pyplot.ylabel('Temperature (K)')
+matplotlib.pyplot.show()
\ No newline at end of file
diff --git a/fortran setup/main.f95 b/fortran setup/main.f95
deleted file mode 100644
index 1be38f6..0000000
--- a/fortran setup/main.f95	
+++ /dev/null
@@ -1,4 +0,0 @@
-program main
-    implicit none
-    write(*,*) "Hello world!"
-end program main